The galaxy appears as an elliptical structure with a smooth, concentrated central bulge. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population dominating the nuclear region. Moving outward from the core, the color transitions slightly toward a redder shade. The lack of defined spiral arms or dust lanes supports its classification as an elliptical galaxy. There is a slight visual distortion in the outer regions, suggestive of a potential minor disturbance. The galaxy appears relatively isolated. The overall morphology indicates a mature system with likely suppressed star formation.
