It seems nearly impossible to get any real info about these things.
It is not difficult to get a rough estimate of the on-axis frequency response (assuming that the half-space
manufacturer driver measurement is reliable) and speaker radiation.
For this we take Tangband's specification (31L, BR @36Hz) and simulate the low frequency response of the speaker with baffle step (orange doted line). Then we use the manufacturer half-space FR measurement and simulate the driver on-axis FR on the speaker baffle and adjust the low FR response.
This gives us approximately the following on-axis FR:
In reality, it should look a bit more even in the low frequency range below 100Hz, as I suspect that some room resonances are included in the manufacturer's measurement.
Because VCAD does not include the cabinet depth in the simulation, its influence on the on-axis FR is missing.
Due to the slim and high cabinet shape of the loudspeaker, a cabinet resonance occurs around 170Hz, which also will have an influence on the on-axis FR, if this resonance is not damped (the same applies to possible BR port resonances).
Since Tangband will make detailed measurements anyway, I will spare myself an time consuming BEM simulation of the speaker to get the radiation and use the simplified simulation in VCAD (normalized hor and ver radiation):
There are a few things to keep in mind when interpreting the radiation simulation.
The influence of the cabinet depth on the radiation is missing, which should slightly change the radiation somewhere around 1kHz.
Above 4-5kHz, the radiation should be less narrow than shown in the simulation, since the driver has a special dust cap that probably takes over the radiation of the high frequencies to a large extent.
I don't know of any off-axis measurements for the CHN-110 driver, but the equally sized, but more expensive, Pluvia 11 has an identical dust cap and shows significantly less beaming than one would expect from a 5.5'' driver.
First manufacturer on-axis measurement, then magazine 0,15,30 deg half-space measurement of the Pluvia 11:

Source:
Klang und Ton 2021-3
Bottom Line: The pronounced on-axis frequency response dip in the range of 2-5 kHz is not likely to be completely flattened off-axis either. This could lead to a rather warm, laid back sound impression. It could also lead to the sound stage being perceived more at height or behind the speakers ("deep sound stage").
The on-axis FR is actually too flat for a full-range driver of this size; one would actually tune to a flat 20°-30° FR. But maybe the special dust cap is sufficient to give a balanced sound impression.