The galaxy appears as a single, centrally concentrated object with a smooth, diffuse light profile. It exhibits a roughly elliptical morphology, showing characteristics of being largely rounded, with no evidence of a pronounced disk or spiral arms. There are no obvious signs of tidal features, mergers, or major disturbances. Color gradients suggest a redder central region, which may indicate an older stellar population or dust obscuration, surrounded by somewhat bluer, less concentrated outer regions. The galaxy's light is generally redder than average.
