The galaxy presents as an elliptical system with a generally smooth, featureless morphology. The light distribution suggests a centrally concentrated bulge, exhibiting a gradual decrease in luminosity outward, and a somewhat ellipsoidal shape. The color gradient appears subtle, with a slightly bluer hue towards the outer edges of the galaxy as well as faint arms near the center, indicating the presence of potentially younger stellar populations in the outer regions. The galaxy does not display any readily apparent signs of major mergers or tidal disturbances.
