The galaxy presents as an elliptical morphology, with a smoothly distributed light profile. The central region appears brighter and more concentrated, exhibiting a yellowish hue, possibly indicative of an older stellar population dominating this area. The outer regions display a bluer tint. There are no obvious signs of spiral arms or significant dust lanes. The shape is somewhat elongated, displaying an aspect ratio that is "in between" round and cigar shaped. Overall, the galaxy shows no clear indication of major disturbances or ongoing mergers, though a minor disturbance can not be ruled out.
