The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. There is little discernible internal structure, no obvious spiral arms, bar features, or prominent dust lanes visible. The light is broadly distributed, indicating a significant bulge component and a lack of intense star formation regions. The galaxy is approximately elliptical, slightly elongated. The overall color suggests a population of older stars, with the light trending towards the redder end of the spectrum. No major tidal features or signs of recent mergers are evident. The galaxy is quite compact.
