Left: radial profiles (in units of HLR) of the stellar mass surface density obtained with base GMe. The results are stacked in seven morphology bins. The error bar in the panel indicates the dispersion at one HLR distance in the galaxies of the Sa bin. It is similar for other Hubble types and radial distances. Right: radial profiles stacked in seven bins of galaxy stellar mass, log M_⋆(M_⊙): 9.1−9.6, 9.6−10.1, 10.1−10.6, 10.6−10.9, 10.9−11.2, 11.2−11.5, 11.5−11.8.