The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The color gradient suggests a relatively old stellar population, with a yellowish hue dominating the core, transitioning to slightly bluer tones at the outer edges. The lack of prominent spiral arms or dust lanes indicates a classification likely leaning towards an early-type galaxy. There is a subtle asymmetry to the outer halo, hinting at a possible past interaction or minor disturbance, though the overall structure remains largely undisturbed. The galaxy exhibits a high degree of central concentration, with the majority of its luminosity emanating from the core region.
