The galaxy presents as an elliptical or lenticular type. It has a smooth, centrally concentrated luminosity profile with a high degree of circular symmetry. There is no evidence of spiral arms or significant disk structure visible at this resolution. The core is a bright, yellow-white hue, suggesting a substantial population of older stars. The outer regions exhibit a bluer color gradient, possibly indicating the presence of younger stellar populations or ongoing, albeit minimal, star formation. No significant tidal features or indications of a major merger event are apparent, though some minor disturbance cannot be ruled out. Overall, it appears to be a relatively quiescent galaxy.
