The galaxy presents a largely smooth, elliptical morphology. It appears predominantly featureless with a centrally concentrated brightness profile. The core region exhibits a warmer color, transitioning to cooler hues in the outer regions. This color gradient indicates potential variations in stellar populations or dust content across the galaxy. There is little evidence of spiral arm structure, and the overall form appears round. There is no visual evidence of a recent or ongoing major merger event or significant tidal disturbances.