The galaxy appears to be a spiral galaxy, observed at a redshift of approximately 0.1. It exhibits a prominent, bright central bulge, surrounded by a disk structure. Faint spiral arms are present, though not sharply defined. The arms appear somewhat flocculent. There is no obvious bar structure visible. The color distribution suggests an older stellar population in the bulge, indicated by the yellowish hue, while the disk shows bluer regions, which could be evidence of ongoing star formation. No major signs of tidal disturbance or ongoing merger activity are apparent. The galaxy seems relatively undisturbed, with smooth outer edges.
