The radial profiles of the stellar mass surface density and ages stacked in seven bins of galaxy stellar mass. In each bin log M(M_⊙) is: 9.2−10.2, 10.2−10.6, 10.6−10.8, 10.8−11.0, 11.0−11.2, 11.2−11.4, and 11.4−11.8. Upper panel: all the galaxies. Middle panel: disk dominated galaxies. Lower panel: spheroidal dominated galaxies (C ≥ 2.8). Here, we show only the profiles in the mass bins with at least two galaxies. Numbers in the middle and lower panels indicate the number of galaxies in each bin. In the upper panel the number of galaxies in each mass bin is 15, except in the highest mass bin which has 17 galaxies. The error bars in all panels indicate the typical dispersion at any given distance in the mass bin log   M (M_⊙) = 11.2−11.4; it is similar for other mass bins and radial distances.