The galaxy presents as a moderately luminous, elliptical morphology. It exhibits a centrally concentrated light profile with a smooth appearance, suggesting a relatively evolved stellar population. The core region displays a yellowish hue, possibly indicative of older stars or dust obscuration. No distinct spiral arms or other prominent features are discernible, supporting its classification as an elliptical galaxy. The overall shape appears close to an elliptical. There is no evidence of strong tidal interactions or ongoing mergers. The observed color gradient suggests minimal ongoing star formation.
