Brightness profile of IRAS 01072+4954 obtained by combining the NIFS (triangles) and 2MASS (squares) data. The H-band profile is shown in the upper panel and K-band at the bottom. In both cases, the dashed line corresponds to a Sersic profile fitted to the bulge, and the dash-dotted line to an exponential function that fits the disk component. The solid lines show the overall fits. The dotted line in the lower panel represents the AGN + hot dust contribution fixed to the 25% of the inner r ≈ 75   pc emission, based on the results presented in Sect. 3.4. The photometric parameters of the profiles in both bands are listed in Table 3.