The galaxy presents a smooth, elliptical morphology. The central region exhibits a high degree of concentration, suggesting the presence of a substantial stellar bulge. The light distribution appears radially symmetric, with a gradual decrease in intensity from the core outwards. There is very little evidence of spiral arm structure or dust lanes, supporting its classification as an early-type galaxy. The galaxy exhibits a mild reddish color, indicating an older stellar population with a lower rate of ongoing star formation. There is no indication of any major mergers or tidal disturbances; however, there appears to be a very small distortion in the outer region of the galaxy. The overall appearance is consistent with a mature, relatively quiescent system that is slowly evolving.
