The galaxy presents as a spiral, observed at a relatively small redshift. Its morphology shows a prominent central bulge, elongated in shape. The galaxy exhibits well-defined, tightly wound spiral arms. No clear bar structure is visible. The color distribution suggests ongoing star formation within the spiral arms. There is no evidence of a major merger, although a minor disturbance is possible. The spiral arm count is difficult to discern, with multiple arms possibly present. The overall disk appears relatively smooth.
