The galaxy presents as a spiral type, with a notably high degree of symmetry in its overall structure. Two spiral arms are clearly visible, originating close to the galactic center and extending outward in a well-defined manner. The arms appear flocculent in nature, displaying clumpy regions that suggest active star formation.

A prominent bulge dominates the central region, exhibiting a moderate concentration of light. There is evidence of a bar feature bisecting the bulge, appearing to add to the overall structure of the galaxy.

The galaxy's disk is observed nearly face-on, allowing for a good view of its spiral structure. The disk appears relatively smooth with a hint of dust lanes associated with the spiral arms. The size of the galaxy is moderate, and there is no indication of any major merger event. There is also no evidence of being an edge-on disk galaxy. Overall, the galaxy presents itself as a well-formed spiral galaxy, actively undergoing star formation within its spiral arms.
