The galaxy presents a primarily face-on orientation relative to our line of sight. It exhibits a pronounced central bulge, appearing as a concentrated region of light that gradually fades outwards. The color of the bulge is distinctly yellower/redder compared to the surrounding disk, suggesting an older stellar population.

The disk component shows hints of spiral arm structure, though these features are somewhat diffuse and not sharply defined. The spiral arms appear to be numerous, with possibly more than two major arms winding outwards from the central bulge. They display a medium winding. The outer regions of the disk transition smoothly into the background sky, indicating a gradual decrease in stellar density. Some bluer regions can be observed along the spiral arms, indicative of recent star formation.

The galaxy appears to have a substantial, moderately luminous disk. There is no evidence of major tidal disturbances or ongoing mergers, although subtle asymmetries within the disk could suggest minor gravitational interactions.
