The galaxy appears as a centrally concentrated, roughly elliptical object. It exhibits a smooth, diffuse light distribution, suggesting it is likely an elliptical galaxy or a lenticular galaxy viewed face-on. There is a slight elongation, but the galaxy is close to circular in appearance. The core region displays a bright, concentrated glow, hinting at a possible active galactic nucleus or a dense stellar population. There is no indication of spiral arm structure or significant dust lanes. The galaxy is primarily composed of older stellar populations as indicated by the predominantly redder color.
