The galaxy presents a primarily elliptical morphology. It exhibits a smooth, diffuse light distribution, with a noticeable elongation along its major axis. A subtle color gradient is observed, transitioning from a bluer hue towards the central region to a redder tint at the periphery. The central region appears brighter and more concentrated, suggesting a higher stellar density or possibly a more active galactic nucleus. There are no prominent spiral arms or distinct dust lanes visible, supporting its classification as an elliptical galaxy. The galaxy appears relatively undisturbed, with no obvious signs of recent mergers or tidal interactions.
