The galaxy presents as a spiral type, exhibiting a prominent disk structure. Spiral arms are readily apparent, and appear tightly wound around the central bulge. The bulge comprises a significant portion of the galaxy's overall luminosity, appearing moderately sized relative to the galactic disk. A bar structure is potentially present, though not distinctly pronounced. The disk itself displays a notable degree of organized structure, with a fairly clear demarcation between the central bulge and the outer spiral arms. No obvious signs of major merging events or significant tidal disturbances are visible. The galaxy is not observed edge-on; instead, a considerable portion of the galactic disk is visible, allowing for the identification of spiral arm morphology. There are likely two main spiral arms.
