The galaxy presents as a lenticular or edge-on spiral type. It exhibits a smooth, elongated profile with a bright central bulge that gradually fades into a fainter disk. There's a slight indication of a more cigar-like shape, with one end slightly more tapered than the other. No distinct spiral arms or prominent dust lanes are visible, consistent with an older stellar population. The overall color appears to be yellowish-white, suggesting a lack of significant recent star formation. There is no visual evidence of any ongoing major mergers or tidal disturbances. The general morphology implies a galaxy that has largely exhausted its gas reserves and is currently undergoing passive evolution.
