This galaxy appears to be a spiral galaxy, observed at a redshift indicating an intermediate distance. Its morphology is disk-dominated, with a relatively small bulge component, or potentially no bulge at all. The spiral arms are quite prominent, loosely wound, and display a flocculent structure. Two main arms are clearly discernible. There is evidence of ongoing star formation within the arms, as indicated by their bluer color. No apparent bar structure is visible at the resolution of the image. The overall structure is somewhat disturbed, possibly indicating a minor gravitational interaction or recent merger event, but the presence of well-defined spiral arms suggests that this galaxy is not undergoing a major merger.
