Global distributions for the galaxy data from the entire 52 cluster sample. Left to right, top to bottom: I‐band apparent magnitude, I‐band absolute magnitude (with Schechter function superposed), rotational velocity width, recession velocity in CMB frame, ratio of semiminor axis to semimajor axis, optical radius, and morphological type in the RC3 scheme (de Vaucouleurs et al. 1991).