The galaxy presents an elliptical morphology, appearing predominantly smooth and lacking any distinct spiral arm structures. The central bulge is prominent, characterized by a high concentration of light, suggesting a large population of older stars. The overall shape is largely in between round and cigar shaped with a slight lean towards being round. There are minor disturbances surrounding the galaxy, which could be indicative of either a past or on-going minor merger event. The lack of strong color gradients suggests a relatively uniform stellar population throughout the galaxy, with no significant regions of active star formation visible in the image. The galaxy’s color is moderately blue, suggesting a relatively young population of stars despite the lack of visible star formation regions. There are no indications of a strong tidal tail or other signs of major disruption.
