The galaxy presents as a disk galaxy, viewed at a high inclination, nearly edge-on from our line of sight. It exhibits a prominent central bulge that appears relatively smooth and concentrated. Dust lanes are visible along the plane of the disk, obscuring the light from stars behind it. These lanes are not uniform, showing patchy distributions. Star formation regions appear present, indicated by diffuse bluish colors along the disk, though are faint, which likely indicates a low star formation rate. There are no obvious signs of a major merger or strong tidal disturbances; however, there might be subtle irregularities or faint plumes that would suggest minor interactions. The disk appears somewhat irregular.
