The galaxy appears as a moderately luminous, elliptical-like structure. It exhibits a smooth, relatively featureless morphology, suggesting a lack of significant ongoing star formation. The central region displays a slightly brighter, more concentrated luminosity profile, potentially indicative of a bulge component. The color gradient seems to shift from a bluer hue near the core to a redder hue in the outer regions. There is no apparent spiral arm structure or prominent dust lanes visible. There is no evidence of strong tidal interactions or major mergers. The object presents with a generally rounded shape, with a very slight elongation.
