The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated light distribution, with brightness diminishing gradually outwards. The overall color appears to be moderately red, suggesting a stellar population that is dominated by older stars and a relatively low rate of ongoing star formation. There is no discernible evidence of prominent spiral arms or a distinct disk structure. The galaxy appears to be generally isolated, without any obvious signs of tidal interactions or major mergers, though subtle disturbances cannot be ruled out. The shape is close to round.
