The galaxy presents as a lenticular or possibly an edge-on spiral galaxy given its elongated, cigar-like shape. The central bulge appears prominent and is characterized by a yellowish-orange hue, potentially indicative of an older stellar population. The disk is visible as a fainter, bluish-white structure extending along the major axis. There is no clear evidence of tightly wound spiral arms, although some subtle variations in the disk's surface brightness suggest the presence of underlying structures. The overall impression is that the galaxy is relatively smooth in appearance, with no significant signs of tidal disturbances or ongoing mergers. However, there are indications of minor disturbances or asymmetrical features in the galaxy's morphology.
