Median stellar intrinsic shape profiles for FRs and SRs as labeled on the right margins. Top panels: triaxiality T(r), bottom panels: axis ratio q(r). Galaxies on the left are divided into stellar mass bins, and galaxies on the right are divided in bins of total in-situ mass fraction. The solid lines show the median profiles, and the shaded regions trace the quartiles of the distributions. Higher stellar masses and accreted fractions correspond to higher triaxiality and less flattened shapes.