The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness moving outward from the core. The galaxy is generally round in appearance with some evidence of a deviation from perfect circularity. There appears to be a slight asymmetry or subtle perturbation in its shape. The overall color is a pale yellow, suggesting a stellar population that is primarily composed of older, redder stars. There is faint evidence of some disturbance around the galaxy, but it is difficult to tell whether this is interaction with another galaxy or part of the galaxy's internal processes.
