The galaxy displays a prominent disk structure, inclined relative to our line of sight. Spiral arms are clearly visible within the disk, demonstrating a two-armed morphology. The spiral arms appear relatively tightly wound. A central bulge is present; its size is moderate compared to the overall size of the galaxy. There is a subtle indication of a bar-like structure crossing the galactic center. No major mergers or significant tidal disturbances are apparent, but there may be some minor disturbance. Overall, the galaxy exhibits features of a spiral galaxy with notable arm structure and a moderate bulge.
