This galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a high degree of central concentration, with a bright core region that gradually decreases in luminosity towards its outer edges. The overall shape is highly rounded, appearing nearly spherical. There is no prominent disk structure or spiral arm features visible. It appears to be a large and very massive galaxy. A very weak level of star formation is estimated. There are no indications of any current or recent major merger events. The galaxy displays a yellowish hue indicating a population of older stars, but it is more blue in the center suggesting that it is also comprised of younger stars. 
