This galaxy exhibits an elliptical morphology, appearing as a fairly smooth concentration of light with a rounded shape. There are no discernible spiral arms or a prominent disk structure. The galaxy appears to be relatively isolated, showing no obvious signs of major interactions or mergers, although a very subtle minor disturbance cannot be completely ruled out. The object displays a centrally concentrated brightness profile. The color index suggests a relatively evolved stellar population within the galaxy. Overall, it likely represents a relatively massive and passively evolving system.
