This galaxy appears to be relatively smooth in structure, with a central concentration of light that diminishes gradually outwards. It exhibits a somewhat elliptical morphology, though it leans towards being rounder than cigar-shaped. The galaxy shows evidence of a redder core region transitioning to more greenish-yellow hues in the outer parts, indicative of varying stellar populations and/or dust content. While there might be slight asymmetries, there is no clear indication of major disturbances from mergers. Based on these characteristics, the galaxy is likely a massive elliptical galaxy with ongoing, but perhaps relatively low levels of star formation.
