The galaxy presents as a centrally concentrated, relatively smooth structure. There is a significant central bulge that is very bright, yellowish, and concentrated. The galaxy displays a gradual decrease in surface brightness as one moves outwards from the core. It appears that the galaxy is generally rounded in shape, but may possibly be slightly elongated. There is no obvious spiral arm structure or strong morphological disturbances visible. The outer regions of the galaxy appear more diffuse and bluer in color than the central bulge. While the galaxy is mostly smooth and round, some minor asymmetries or faint features may exist, especially at the outer edges of the object. Overall, the galaxy is suggestive of an elliptical type with moderate star formation.
