The galaxy presents as a relatively compact object with an apparent flattened, elliptical morphology. The central region exhibits a higher surface brightness, indicating a possible concentration of stars or active galactic nucleus. Fainter, more diffuse emission extends outwards from the core, displaying a slightly irregular shape. There is evidence of a disruption in the shape, with a slight extension in the right region of the galaxy. The color appears relatively uniform across the galaxy, with a slight reddening towards the edges. Overall, the galaxy shows signs of potential interaction or internal disturbances, though it remains mostly intact and is not in the process of major merging. 
