The galaxy presents as a relatively smooth, centralized structure. It appears to be elliptical in shape, though tending toward a rounded morphology. The light distribution suggests a high degree of concentration toward the center, with a bright, well-defined core. There is a distinct color gradient from the central region outwards; the core exhibits a bluer hue, transitioning to redder tones in the outer regions of the galaxy. No prominent disk-like structure, spiral arms, or obvious dust lanes are visible. There are no indications of tidal tails or major disturbances, suggesting it is not undergoing a major merger event.
