Radial profile of the NGC 1015 galaxy in 3.6 and 4.5 μm-bands modeled with the IRAF ellipse task, denoted as blue and red points, respectively. Overplotted are orange crosses from Muñoz-Mateos et al. (2015) for the 3.6 μm-band. For clarity, only composite models are given for 3.6 μm (black) and 4.5 μm bands (gray), that correspond to the sum of all individual subcomponents. Individual subcomponents are presented only for the 3.6 μm band (point spread function, bulge and disk).