The galaxy exhibits an elliptical morphology, appearing somewhat flattened. A bright, concentrated central bulge is evident, possibly indicating a supermassive black hole. Surrounding the bulge is a disk component, displaying a blue-green color gradient suggestive of ongoing star formation. The galaxy's periphery shows hints of disturbances or tidal features, potentially indicative of a past or ongoing minor merger event. There are no prominent spiral arm structures visible. The overall smoothness suggests it is likely an early-type spiral or lenticular galaxy, with possible interactions influencing its structure.
