The galaxy presents a generally elliptical morphology, appearing quite smooth in texture with a high degree of circularity. A dominant central bulge exhibiting a yellowish-orange hue suggests a significant population of older stars, possibly indicative of a relatively quiescent star formation rate. The overall color profile hints at a galaxy with a substantial mass, where star formation has either slowed considerably or is concentrated in specific regions not readily apparent in this image. There is a possible faint, disturbed feature to the left of the galaxy which could be either a feature of the galaxy itself or a nearby interacting galaxy.
