The galaxy presents as a face-on spiral galaxy with a noticeable central bulge. The spiral arms are somewhat diffuse and flocculent, rather than well-defined, suggesting ongoing but not particularly intense star formation. The galaxy appears relatively smooth, indicating a mature system that is potentially evolving towards a more lenticular or elliptical morphology. There is evidence of minor disturbances in the galactic disk, likely caused by past interactions or mergers. Overall, it appears as a typical spiral galaxy undergoing a quiescent period of star formation with some signs of past interactions. The galaxy emits light across the g, r, and z bands, suggesting a range of stellar populations.
