The galaxy exhibits a generally smooth morphology, though there are some indications of possible disturbances or features. It is elliptical in shape, appearing more round than elongated. The central region displays a high surface brightness, indicating a concentrated distribution of stars. There is a color gradient across the galaxy, with the central region appearing redder, and the outer regions displaying slightly bluer hues. The redder core could be due to the presence of older stellar populations or dust obscuration, whereas the bluer regions indicate younger stellar populations. The overall reddish color suggests that this galaxy may be a relatively quiescent system, with limited ongoing star formation. There is a hint of interaction or merger. The data hints that this is a large, very massive galaxy.
