The galaxy appears as a centrally concentrated, elliptical-like system with a smooth overall morphology. It exhibits a gradual decrease in surface brightness from the core outwards. The central region has a yellowish-white hue, suggesting a population of older stars. Fainter, reddish-tinged features or possibly a faint disk-like structure are weakly evident, extending along the horizontal axis, though these are not sharply defined. No strong signs of recent or ongoing major merger events are visible; however, there is a slight asymmetry in the outer isophotes that hint at minor tidal disturbances. Based on the color and morphology, it is likely a relatively massive system, perhaps a lenticular or early-type spiral galaxy with suppressed star formation.
