The galaxy appears as a concentrated, elliptical-like structure. The light is centrally condensed with a smooth distribution, lacking any discernable spiral arm features or obvious dust lanes. The color gradient indicates a central concentration of older stars as indicated by the redder hue. The outer regions exhibit a gradual decrease in luminosity, with a faint greenish cast suggesting some presence of younger stars. There is no indication of a recent major merger event, tidal tails or any strong interactions with neighbor galaxies, however, there are possible indications of a minor disturbance based on the irregular outer morphology. The round shape, smooth features, and color profile suggest that this galaxy is likely an evolved system with a relatively low star formation rate.
