The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity outwards. The color appears to be a red-shifted orange, suggesting a population of older stars and a relatively low current star formation rate. There is no apparent disk structure or spiral arms. No signs of major disturbances or tidal features are visible, suggesting it is not undergoing a major merger. It is a gravitationally mature system.