The object is a galaxy, likely at a considerable distance. The galaxy's light exhibits a significant redshift.

Morphologically, the galaxy appears to be relatively smooth, with little evidence of spiral arms or a prominent disk structure. The galaxy is elliptical, with a slight deviation from perfect circularity.

There is evidence of possible tidal interactions or mergers with smaller satellite galaxies. There are hints of disruptions in the outer regions of the galaxy, which may be indicative of ongoing or past mergers.