The galaxy presents as a relatively compact, elliptical-like structure, displaying a smooth, featureless morphology. It appears to be largely spheroidal with intermediate roundness. The color gradient suggests a redder overall population, indicative of older stars with minimal ongoing star formation. There are no readily apparent signs of spiral arms or a prominent disk. The absence of strong tidal features suggests it has not experienced any recent major mergers. There is a possible very minor distortion of the galaxy at the upper left side of the ellipse, this could suggest a minor merger.