The galaxy presents as an inclined, rotating disk galaxy. The disk appears to be primarily viewed edge-on, with a distinct central bulge.

The bulge region exhibits a smooth, concentrated luminosity profile, indicating an older stellar population. There appears to be a ring of material around the bulge. Dust lanes are observed along the periphery, contributing to the edge-on appearance of the disk. These lanes partially obscure the light from stars behind them, revealing the dusty nature of the galactic plane.

The disk of the galaxy has notable features, including a section that is visibly disrupted and distorted from the primary structure of the disk on the lower left side of the galaxy. This may indicate a recent gravitational interaction, and perhaps the early stages of a galactic merger. The disturbed area presents as a diffuse, elongated feature extending away from the main disk, displaying an unusual shape.

The overall color distribution in the galaxy suggests a gradient from older stellar populations in the bulge to younger, bluer star-forming regions in the disk and in the region of disruption.
