The galaxy appears to be a relatively smooth, elliptical type. It exhibits a high degree of circularity, appearing nearly perfectly round. There is no obvious spiral arm structure. The central bulge dominates the overall morphology, with a gradual decrease in luminosity extending outwards. The color profile suggests an older stellar population, potentially with a lack of ongoing star formation. No significant dust lanes or tidal features are apparent. The galaxy appears isolated and undisturbed.
