The galaxy appears to be a luminous elliptical, exhibiting a smooth, concentrated light profile indicative of an older stellar population. The galaxy core is bright and gradually fades into the outer regions, which have an overall ellipsoidal morphology. There is no obvious presence of spiral arms or a prominent disk component. The color is somewhat uniform, with a slight reddening toward the central region. It is a fairly large galaxy. No signs of active galactic nuclei (AGN) activity, such as jet-like structures or strong emission lines, are apparent in this imagery. There are no signs of mergers or tidal tails visible.