The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a yellowish-white color gradient, indicating a population of older stars. Fainter, bluer, regions with diffuse edges are located near the central region, indicating some low level of recent star formation. No distinct spiral arm structure is discernible. The galaxy appears relatively isolated and unperturbed, without any obvious signs of tidal interactions or major mergers. Based on the observed morphology, this is likely a massive, evolved galaxy with little active star formation.
