The observed galaxy presents as a spiral type, exhibiting a prominent disk structure. The disk is viewed at a slight inclination. Spiral arms are evident, although not exceptionally well-defined. There is no evidence of a strong central bar structure. The central bulge is moderately pronounced.

The overall color of the galaxy is suggestive of ongoing star formation, with a bluish tint noted within the spiral arms. There is no significant evidence of major disturbances or mergers, but a possible minor disturbance is present. The galactic core is a yellowy color, and the galaxy appears relatively smooth in nature.
