The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge dominates the structure, exhibiting a yellowish hue indicative of an older stellar population. Fainter, bluer regions are observed in the outer regions, perhaps indicative of ongoing star formation. The galaxy appears mostly undisturbed, with no signs of major mergers or tidal disruptions. There is a slight asymmetry in the light distribution, potentially suggesting a minor interaction or internal process. Overall, the galaxy exhibits characteristics consistent with a massive elliptical galaxy with a moderate amount of star formation in its outer regions.
