The galaxy presents a largely smooth, elliptical morphology. It exhibits a diffuse, centrally concentrated luminosity profile, with a gradual decline in brightness from the core outwards. There is minimal evidence of spiral arm structure or prominent dust lanes, suggesting a relatively evolved stellar population. The overall color is consistent with an older stellar population, though some bluer components exist. These colors could be indicative of ongoing low-level star formation. There does not appear to be any evidence of a major ongoing merger, though some subtle distortions cannot be ruled out, possibly indicating minor past interactions. The galaxy's apparent shape leans toward being in between round and elongated.