This galaxy exhibits a flattened, disk-like morphology indicative of a spiral galaxy. The central bulge appears relatively small. The spiral arms are tightly wound. There is no evidence of a strong bar structure bisecting the bulge. The overall color suggests a mix of stellar populations and a moderate degree of ongoing star formation. There are no obvious signs of a major merger or significant tidal disturbances. The outer regions appear relatively smooth, suggesting a well-defined disk with minimal recent interaction.
