The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a bright, concentrated core that gradually diffuses outwards. There is a clear lack of prominent spiral arm structures or a defined disk. The galaxy appears primarily spheroidal in shape with a high degree of roundness. Subtle color gradients are visible, suggesting potential variations in stellar populations or dust content within the galaxy. There is no obvious evidence of tidal tails, ongoing mergers, or major disturbances in its overall structure.
