The galaxy presents as a lenticular or edge-on spiral galaxy. It exhibits a smooth, elongated profile with a central bulge that appears bright and concentrated. The visible color gradient suggests a concentration of older stars in the central bulge, which transitions to slightly bluer hues towards the outer regions of the disk. The lack of clearly defined spiral arms indicates a relatively low rate of recent or ongoing star formation. No signs of major mergers or tidal disturbances are apparent in this image. The galaxy appears generally undisturbed and relatively isolated.
