The galaxy presents as a relatively smooth and elliptical structure. It exhibits a concentrated central bulge that appears significantly brighter and more yellow than the surrounding regions. There is a lack of apparent spiral arm structure or prominent dust lanes. The galaxy appears nearly circular with a slightly elongated shape. The outer regions of the galaxy appear to fade gradually, lacking a sharp defined edge. There are no signs of major tidal disturbances or ongoing mergers, although a possible minor disturbance cannot be entirely ruled out.
