The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated brightness profile that gradually fades outwards. The overall color appears to be slightly redder, indicating an older stellar population and potentially lower levels of on-going star formation. There may be a slight indication of a disk-like structure, but it is predominantly smooth. There is no obvious evidence of tidal features or other strong interactions with neighboring galaxies, although minor disturbances cannot be ruled out. It appears relatively undisturbed and exhibits a shape that is closer to round rather than elongated.
