Kinematic and structural properties of type I (circles), type II (triangles), and type III (crosses) galaxies in the h_R–M_⋆ plane. From left to right, the data points are color-coded by the ratio of break radius to inner disk scale length R_break/h_R, rotational support κ_rot, stellar halo mass fraction f_halo, and ex situ stellar mass fraction f_ex-situ. In each panel, the symbol size scales with the corresponding color-coded quantity. The gray dashed, gray dotted, and black solid lines represent the linear fits to the h_R–M_⋆ relation for type I, type III, and the total disk sample, respectively; shaded regions denote the 1σ fitting uncertainties. The error bars indicate the standard deviation of the residuals from the global linear fit.