This galaxy exhibits a clear spiral morphology. The spiral arms are well-defined and appear relatively tightly wound. There is evidence of two dominant spiral arms. A moderate bulge is apparent, although it does not dominate the overall structure of the galaxy. There is no strong bar structure visible, although a weak bar may exist. The galaxy appears to be undergoing active star formation, as indicated by the presence of blue regions within the spiral arms. No major merger events are indicated, though a minor disturbance or interaction cannot be completely ruled out based on this image alone. The overall disk structure is not edge-on, presenting a face-on view of the galaxy's spiral pattern. The disk appears relatively smooth overall, but some features are apparent along the spiral arms.
