The galaxy appears to be a spiral galaxy, observed face-on. It exhibits a central bulge, and spiral arms emanating outwards. The bulge displays a yellowish-white hue, suggesting a population of older stars. The spiral arms are moderately wound and appear to be dominated by two prominent arms. Patches of blue are observed throughout the arms indicating regions of active star formation. Overall, the spiral structure reveals a grand design, though some asymmetry is apparent, likely due to gravitational interactions or uneven distribution of gas and dust. No major merger events are apparent.
