The galaxy exhibits a disk-like morphology, presenting with a noticeable inclination relative to our line of sight. The central bulge is relatively small and not particularly prominent, with a brightness less than the disk. Evident spiral arm structures extend from the central region, loosely wrapping around the galaxy. These arms appear somewhat flocculent rather than tightly wound. Dust lanes or patchy regions are interspersed within the spiral arms.

The overall color gradient suggests potential variations in stellar populations across the galaxy, as evidenced by the color differences in the disk and spiral arms. There are slight signs of asymmetry in the spiral arm structure. While the galaxy appears relatively isolated, a potential tidal stream is not visibly discernable. The disk is the dominant feature, with the bulge contributing minimally to the overall light. The light from the galaxy is mostly homogenous in nature with minimal irregularities.
