The object appears to be a spiral galaxy at a moderate redshift. It presents a somewhat disturbed morphology, with strong evidence of ongoing interaction or a past minor merger event. The spiral arms are prominent but lack grand design coherence. The arm structure appears flocculent, exhibiting regions of intense star formation that give the arms a clumpy appearance. The winding of the spiral arms is intermediate, neither tightly wound nor completely open. A small bar structure may be present, but it is not the dominant feature of the galactic morphology. The bulge is moderate in size relative to the disk, though it is difficult to delineate its precise boundaries, suggesting it is neither exceptionally large nor small. Overall, the galaxy demonstrates active star formation and has been subject to some form of gravitational disturbance, impacting its structure and evolution.
