The galaxy presents as a compact, relatively bright object. It is likely a distant galaxy based on its small angular size. 

The central region appears to be smooth and somewhat amorphous. The galaxy exhibits a generally elliptical shape, with no obvious spiral arms or disk structures visible. There may be some signs of tidal disruption, but the feature appears unclear given the resolution. 

Color gradients exist across the galaxy. The central region exhibits a bluer hue, possibly indicative of ongoing star formation or a more luminous active galactic nucleus. Moving outwards from the center, the galaxy transitions to a greener color, possibly due to older stellar populations.
