The galaxy presents an elliptical morphology. It exhibits a smooth, centrally concentrated light distribution, with a gradual decline in luminosity towards the outer regions. The central region appears to be brighter and potentially contains an older stellar population. The overall color gradient suggests a redder core transitioning to a slightly bluer halo, possibly indicating ongoing, but low-level, star formation in the outer regions. There is no apparent evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, with no indications of major recent mergers or tidal interactions. Its shape is close to round.
