The object exhibits characteristics of a galaxy at a considerable distance, inferred from its observed redshift. Morphologically, the galaxy presents a complex structure. A significant portion of the light seems to originate from a feature that could be a central bulge or a smooth, unresolved component. However, the image suggests the presence of a disk.

There appears to be ongoing interaction or merging events. Some parts show disturbed shapes, suggesting minor gravitational interactions or recent mergers. The color distribution indicates a mix of stellar populations, with possible regions of active star formation implied by the bluer colors. Other regions contain more evolved stars. There is no definitive evidence of a spiral arm structure.
