This galaxy exhibits a clear disk structure with prominent spiral arms. The arms appear tightly wound around a central bulge. The bulge is moderately sized, not appearing overly dominant. The spiral structure suggests a two-armed configuration is likely. The overall color suggests active star formation is present within the disk, particularly in the spiral arms, which appear slightly bluer. There is evidence of a bar structure within the central region, but the arms are not as extended. No major distortions are present, indicating no ongoing major merger events, although there may be some minor disturbances.
