Synoptic view of the Sérsic indices of the galaxies from NIR to NUV bands. NIR and optical Sérsic indices are obtained from the fit of the luminosity profiles of the CGS (Ho et al. 2011; Li et al. 2011), except for NGC 1366, NGC 2685, and NGC 3818, which are not included in that catalog. For these galaxies we used UVOT U, B, and V bands. The morphological type, T, is taken from Hyperleda, as reported in Table 1. The arrows indicate the r^{1 / 4} law.