The galaxy presents as a luminous, elliptical-like object with a smooth, relatively featureless morphology. It exhibits a concentrated core region that gradually diffuses outwards. The color profile appears to shift from a slightly yellow-white hue in the center to a more neutral white in the outer regions, suggesting a population of older stars. While the overall structure seems undisturbed, closer inspection reveals hints of minor asymmetries. There is no discernible spiral structure or significant dust lane. The galaxy does not appear to be undergoing a major merger or significant tidal interaction with another galaxy. The object's roundness is high, with a shape trending away from cigar-shaped or disk-like morphology. 
