The galaxy appears as a centrally concentrated, elliptical-like structure with a smooth overall morphology. There is a prominent, bright core that gradually fades into the outer regions of the galaxy. The galaxy exhibits a slightly elongated shape. The color profile suggests a population of older stars, indicated by the reddish-yellow hue that is most prominent in the center. No distinct spiral arm structures or significant dust lanes are discernible in the image. There are no obvious signs of ongoing major mergers or tidal disruptions affecting the overall structure.
