The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that is bright and yellowish-orange in color, suggesting an older stellar population. The overall shape is nearly circular, with a slight deviation towards a more elliptical form. There is a faint, diffuse halo surrounding the central region, which gradually fades into the background. There is very little evidence of spiral arms or significant dust lanes. The galaxy seems to be relatively undisturbed, with no obvious signs of a recent major merger or tidal interactions. The red color in the halo suggests that there has been a small amount of recent star formation. 
