The galaxy presents a largely smooth, elliptical morphology. The light profile exhibits a central concentration that fades gradually outwards, suggesting a relatively old stellar population. The galaxy is approximately round in shape. There is no clear evidence of spiral arm structure or significant dust lanes. No prominent tidal features, such as streams or shells, are apparent, suggesting the galaxy has not recently undergone a major merger. There is no evidence of a strong active galactic nucleus in this image. The color is generally redder, suggestive of older stars and lower star formation rate. There appear to be some minor disturbances in the galaxy's structure, which may indicate a small interaction with another galaxy.