The observed galaxy presents as a spiral galaxy, with a redshift indicating considerable distance. The galaxy's structure is characterized by a prominent central bulge that appears moderately sized. Faint spiral arms extend from the central bulge, exhibiting a tightly wound morphology. The spiral structure seems to be multi-armed.

There is evidence of active star formation present in the galaxy, particularly within the spiral arms, as indicated by the subtle color variations. No bar feature appears to be present. There does not appear to be any major mergers or disturbances, though the outer regions are not as clear.
