The galaxy presents an elliptical morphology, elongated along its major axis. The central region exhibits high surface brightness, appearing almost unresolved and quite concentrated. The color of the central region is notably bluer compared to the outer regions, indicating the potential presence of younger stellar populations or active galactic nuclei activity. A faint, reddish ring is visible surrounding the central blue core, potentially indicative of older stellar populations or dust absorption. The outer regions of the galaxy are fainter and appear more diffuse, transitioning gradually into the background sky. There are hints of possible tidal features or faint streams extending from the galaxy, suggesting potential past or ongoing interactions with other galaxies. The overall structure appears moderately disturbed, potentially influenced by minor gravitational interactions or internal dynamics. 
