The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region displays a bright, intense luminosity, suggesting a high density of stars and possibly the presence of an active galactic nucleus. The outer regions gradually fade in brightness, showing a diffuse halo with little visible substructure. The overall color is slightly blueish, indicative of ongoing star formation, though not at an extremely vigorous rate. There is no prominent spiral arm structure or dust lanes discernible in the image, further supporting the classification as an elliptical galaxy. The shape is generally round, with only a slight elongation visible. There is no visual evidence of any major mergers or tidal disturbances affecting the galaxy's structure.
