This galaxy appears to be a relatively smooth, elliptical type. It has a centrally concentrated light profile, with a gradual decrease in brightness towards the outer edges. The galaxy's overall shape is somewhat rounded. There appears to be a subtle hint of a disk component, but it is not clearly defined. The color suggests a stellar population that is relatively old, with limited ongoing star formation. There are no signs of strong tidal features or major disturbances, indicating that it is likely not undergoing a major merger. There might be some minor disturbances, or a hint of a faint plume, but it is difficult to say for sure.
