Comparisons of the stellar kinematics measured from the NIRSpec G235H/F170LP observations and a range of JAMs. The black line shows the model with a constant M/L_F814W, and colored lines the models that incorporate a radially varying M/L_F814W plus 1σ error. The dashed vertical line marks the extent of the SMBH’s SOI. The data profile was obtained by averaging over circular annuli, and the associated errors are defined as the median of the V_rms uncertainties calculated by PPXF (i.e., ΔV and Δσ) of all bins within the circular annuli.