The galaxy presents as a spiral galaxy, exhibiting a distinct disk structure. The arms are clearly defined, wrapping moderately around a central bulge. The central bulge appears prominent, displaying a concentration of light. Two spiral arms are dominant. The spiral arms show variations in intensity, suggesting differing stellar populations or dust lane obscuration. There is no bar feature. There is a small object to the left of the galaxy, likely a dwarf galaxy or star cluster undergoing a minor merger. The galaxy is not perfectly edge-on; it's inclined.
