This galaxy appears to be a relatively smooth, elliptical galaxy. It presents with a dominant, centrally concentrated bulge exhibiting a yellowish hue, indicating a significant population of older stars. The overall shape is roughly circular. There's no discernible spiral arm structure or prominent dust lanes visible in the image. No significant signs of ongoing merging activity or major disturbances are apparent, suggesting it is a relatively relaxed system. The galaxy's estimated size is relatively compact. Given the observed color, we can infer low to moderate star formation activity.
