Two examples for the 2D surface brightness modeling of i-band images reconstructed from MUSE. Top panels: broad-band image extracted from the MUSE cubes covering for the i-band. Middle panels: best-fit 2D surface brightness model determined with galfit, which consists of a PSF for the AGN and two Sersić components for the host galaxy. Bottom panels: residuals of the best-fit model which highlights the substructure of the galaxies such a spiral arms, but also foreground stars, companions and background galaxies are visible. Those features are masked out during the fitting as shown by the shaded areas.