The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge, indicating a high stellar density in the core region. The galaxy's light profile is characterized by a gradual decrease in intensity from the center outwards, suggesting an aging stellar population. The galaxy is elongated, with an apparent lack of spiral arms. The overall color appears to be redder or yellower, possibly indicating older stars and a low ongoing star formation rate. There are no readily apparent signs of significant dust lanes or prominent star-forming regions, which further supports the idea of a relatively quiescent galaxy with a significant fraction of smooth morphology.
