The galaxy presents as a spiral galaxy with a notable disk structure. Evidence of spiral arms is visible, appearing somewhat fragmented and loosely wound. The central bulge is moderately sized and displays a yellowish-orange hue, suggesting an older stellar population. The disk exhibits a bluer color, indicative of ongoing star formation. There are areas of enhanced brightness within the disk, likely corresponding to star-forming regions. Overall, the galaxy appears relatively undisturbed with no obvious signs of a major merger event, though some minor disturbance cannot be ruled out. The galaxy is observed at a redshift indicating a considerable distance.
