The galaxy presents a primarily smooth, elliptical morphology. The main body exhibits a notable central bulge, characterized by a concentrated region of higher luminosity. This central region appears more red-shifted, suggesting an older stellar population or significant dust obscuration. The overall shape appears slightly oblate. There is faint greenish-blue color toward the outer edges of the galaxy. The outer edges are quite diffuse, suggesting a gradual decline in stellar density. There is no indication of spiral arm structures or a prominent disk. No signs of tidal tails or interactions with other galaxies are visible. Overall, the galaxy appears to be an isolated, relatively undisturbed system.
