The galaxy presents as a spiral type, displaying distinct, well-defined spiral arms. The arms exhibit a tightly wound morphology, appearing closely wrapped around the galactic center. A modest central bulge is discernible, though it does not dominate the overall structure. The galaxy's disk is observed face-on, allowing for a clear view of its spiral structure. No prominent bar feature is apparent within the galactic center. Indications suggest that the galaxy is not currently undergoing a major merging event. The color profile suggests moderate star formation activity.