The galaxy appears to be a relatively smooth, elliptical galaxy with a somewhat spheroidal shape. It exhibits a strong central bulge, characterized by a high concentration of light. The galaxy’s color gradient suggests a population of older stars, particularly concentrated in the core, giving it a yellowish to reddish hue. There are hints of possible tidal features or disturbances, suggesting a potential interaction or merger in its past. Based on its apparent lack of significant spiral arms or dust lanes, this galaxy is likely to be classified as an early-type galaxy with a moderate mass. Its overall structure seems largely undisturbed, hinting that any past interactions were not recent or highly disruptive.
