Running mean as a function of radius of the azimuthally averaged profiles of the stellar velocity dispersion (upper left panel), inclination-corrected specific angular momentum (upper right panel), age (lower left panel), and metallicity (lower right panel) for the sample galaxies in three different mass bins: 8.9 ≤ log(M_*/M_⊙) ≤ 10.5 (blue symbols), 10.5 <  log(M_*/M_⊙) ≤ 10.8 (green symbols), and 10.8 <  log(M_*/M_⊙) ≤ 11.2 (magenta symbols). The dashed vertical lines mark the position of the average transition radius R_tr, 1 for each mass bin. The dash-dotted lines represent the fits to the metallicity gradients in the two regions defined by transition radii R_tr, 1 and R_tr, 2. The error bars trace the dispersion of the points around the mean trend. The radial profiles of the stellar kinematics and population properties of the three edge-on galaxies, FCC 153, FCC 170, and FCC 177, have been excluded from the mean.