The galaxy presents as a centrally concentrated object with a largely smooth, elliptical morphology. It exhibits a bright, relatively compact core that appears to fade gradually into the surrounding galactic halo. The overall color appears to be moderately red, suggestive of an older stellar population, but with some bluer regions towards the outer edges, which could indicate some ongoing, albeit moderate, star formation. No prominent spiral arm structures or significant dust lanes are readily apparent in the image. The galaxy's shape tends toward roundness rather than being highly elongated. There is no clear evidence of major disturbances or ongoing merger activity, though subtle asymmetries in the outer regions could suggest past interactions. Overall, the galaxy appears to be a relatively isolated, evolved system.
