Radial variation in the Σ_M⋆ (top), Σ_SFR (middle), and sSFR (bottom) of strong and weak AGN based on their X-ray strength compared to the SF sample. The profiles of strong X-ray AGN with log Lx_{2 − 10 keV} > 41 erg s⁻¹ are shown with purple lines, moderate X-ray AGN with log Lx_{2 − 10 keV} < 41 erg s⁻¹ with red lines, and AGN without Lx_{2 − 10 keV} detection with green lines. The profiles of SF samples are shown with black lines. This figure shows that strong X-ray AGN exhibit a profile similar to that of the SF sample, whereas weaker X-ray AGN show signs of quenching in the center and enhancement in the outer region of galaxies. Error bars represent the 3σ confidence intervals.