This galaxy presents a generally smooth, elliptical morphology. It appears to be relatively undisturbed, showing no strong evidence of a recent major merger. The central region exhibits a concentrated brightness, suggesting a possible bulge. Moving outward from the core, the galaxy's luminosity gradually decreases with a faint extended halo. The overall color profile indicates a dominant population of older stars, contributing to the galaxy's redder appearance. There is some evidence of minor asymmetry and/or a faint disk structure that would indicate later type morphology. There appears to be a relatively smooth distribution of light across the galaxy, rather than patchiness that would indicate more active star formation.
