The galaxy presents as an elliptical morphology, displaying a smooth, centrally concentrated light profile. There is no obvious spiral arm structure or bar feature. The galaxy exhibits a moderate degree of ellipticity, appearing more in-between round and cigar-shaped. There is little evidence of ongoing major mergers or significant tidal disturbances affecting the galaxy's structure. The overall color suggests a relatively evolved stellar population. The galaxy appears to be relatively isolated within its immediate environment.
