Surface brightness profiles in the H band (left panels) and in the I band (right panels) for three systems illustrating the different galaxy morphologies in our sample: the early-type galaxy 19195 (top panels), the barred late-type galaxy 13942 (middle panels), and the late-type galaxy 21796 (bottom panels). The results from single- and multi-component Sérsic models are shown in violet and green, respectively. Black points represent the observed surface brightness profile; solid lines show the models convolved with the PSF; dashed lines stand for the decomposition of the multi-component model into bulge (red), disk (blue), and bar (orange); dotted vertical lines represent the effective radius; and the dotted gray vertical line is the van der Wel et al. (2012) (single Sérsic) effective radius. We display the galaxy stamp in units of surface brightness (mag arcsec⁻²; see the horizontal color bar beneath each map) with shadowed areas matching the masks used to obtain the observed light profile, the galaxy ID in the top left corner, and a scale bar in the top right corresponding to 10 kpc.