The galaxy appears to be a relatively small and faint object, likely at a significant distance given its redshift. It exhibits a generally smooth morphology, but not perfectly elliptical. The shape seems to be somewhere between a disc-like or spheroidal galaxy. The central region displays a higher surface brightness, possibly indicating a more concentrated stellar population or active galactic nucleus. There appears to be slight asymmetry or minor disturbances in the galactic structure, indicating a possible interaction or recent minor merger event. There is a bluer color in the central and outer edges of the galaxy, which may indicate some star formation occurring, even though the galaxy is overall a relatively quiescent system. There is some visual evidence suggesting the faint presence of spiral arms.
