The galaxy appears to be a relatively smooth, elliptical galaxy. It has a centrally concentrated, bright core that gradually diffuses outward into a fainter halo. The color profile suggests an aging stellar population, with a yellowish-orange hue dominating the central region. There is a subtle color gradient, transitioning to slightly bluer tones in the outer regions, hinting at the presence of younger stars at the periphery. There is no apparent dust lane or spiral arm structure. The morphology suggests that the galaxy is in a relatively relaxed state. There appears to be a very minor disturbance in the shape of the galaxy.
