Dependence of physical parameters of our target galaxies in the samples of C1−C3 on the clustercentric radius: (left) (u − r), (middle) SFR, and (right) Δ(g − i). Median curves are drawn for the cases of early-type AGN host galaxies (filled circle and solid line), early-type non-AGN galaxies (filled square and solid line), late-type AGN host galaxies (open circle and dotted line), and late-type non-AGN galaxies (open square and dotted line). Late types with axis ratio of b/a < 0.6 are eliminated. SFRs are computed with H₀ = 70 km s^-1 Mpc^-1 and Salpeter IMF.