The galaxy presents a somewhat elongated, though largely amorphous, structure. Its color profile indicates an overall red hue with slightly yellower areas, which might suggest an older stellar population and subdued star formation activity. The galaxy appears relatively compact, with a smooth brightness distribution but some evidence of faint, diffuse extensions in the periphery. There is a slight indication of minor tidal disturbances or interactions that have disturbed it. The internal structure displays a hint of complexity, potentially with a central bulge embedded in a more extended disk-like component. Given its redshift, the galaxy is situated at a considerable distance, and its morphology is likely influenced by gravitational lensing. The galaxy does not appear to be undergoing major mergers but possibly experienced minor ones.
