This galaxy appears as a moderately bright object with a generally elliptical morphology. It displays a smooth, concentrated central bulge that dominates the overall light profile. A faint, diffuse disk is suspected, but its presence is not definitively confirmed due to its low surface brightness and subtle features.

There is no clear evidence of spiral arm structure or significant dust lanes within the galaxy. The galaxy's color suggests a relatively evolved stellar population, likely dominated by older stars. The galaxy exhibits a mild degree of elongation. There is no indication of a major ongoing merger event, though some minor disturbances are possible.
