The galaxy presents as a face-on spiral structure. It exhibits a central bulge with a yellowish hue, suggesting a population of older stars. Fainter spiral arms extend outwards from the bulge, displaying a bluish tint indicative of ongoing star formation. These arms appear somewhat tightly wound. No significant bar structure is apparent. There is a slight indication of some asymmetry or minor disturbances. The galaxy has an estimated size of approximately 8.6 kpc.
