The galaxy presents as a relatively small, edge-on spiral. The central bulge appears prominent and has a somewhat rounded morphology. The disk of the galaxy is clearly visible, with a high inclination relative to our line of sight. There is a hint of dust lane absorption along the plane of the disk, contributing to the overall redness. There is some light emanating from the surrounding halo region. There may be a small tidal stream extending from the top of the galaxy. The galaxy shows no strong signs of a major merger or significant disturbance.
