The galaxy presents as an elongated, disk-like structure, likely an edge-on or nearly edge-on spiral or lenticular galaxy. The central bulge is prominent and appears relatively smooth and concentrated. The overall color is yellowish, suggesting a population of older stars and a lower rate of ongoing star formation across the galaxy. There is a hint of a darker dust lane or obscuration visible along the galactic plane, further supporting the interpretation of a disk galaxy viewed at a high inclination. There is some asymmetry in the outer disk of the galaxy. This may be due to a warp in the galaxy. There are no prominent spiral arms readily discernible.
