The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile with a gradual decrease in surface brightness towards its outer regions. There is minimal evidence of spiral arms or significant disk-like features; the galaxy appears largely spheroidal. The dominant color is a reddish-yellow hue, which implies an older stellar population with relatively low current star formation. The overall shape is generally round. There is very little evidence of any major interactions or ongoing mergers. There may be a small satellite galaxy nearby.