The galaxy presents as a spiral, viewed at an angle relatively close to face-on. The central bulge is small and shows a yellowish color, indicating a population of older stars. The spiral arms are tightly wound, and have a bluish color, suggestive of active star formation. Three primary spiral arms appear to emanate from the central region, with some branching and fragmentation visible along their lengths. There is no indication of a strong bar structure. Overall, there is no significant indication of merging or major disturbance; however, a slight asymmetry could indicate minor interaction in the past. The galaxy appears relatively compact with an estimated effective radius around 4 kpc.
