The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a central bulge that is concentrated and appears yellowish-orange in color, suggesting an older stellar population. The outer regions are less defined, with a gradual decrease in luminosity. The faint, diffuse nature of the outer regions suggests a lack of significant ongoing star formation in the disk, consistent with a more evolved galaxy. There's a hint of slightly bluer color in some very faint, outer sections, possibly indicating a low level of recent star formation. Overall, the galaxy appears isolated and undisturbed, showing no strong signs of tidal interactions or major mergers.
