The galaxy presents as an elliptical morphology, appearing mostly smooth with a high degree of central concentration. The color gradient suggests an older stellar population, with a yellowish-orange hue prominent towards the core and a subtle blue tinge in the outer regions, potentially indicative of some recent, low-level star formation. The galaxy appears elongated, with a ratio of approximately 2:1, which indicates moderate ellipticity. There appears to be little in the way of disk structure or significant tidal features, and the overall appearance suggests a relatively undisturbed system, with no obvious signs of recent major mergers or interactions. It is moderately luminous and fairly massive based on the apparent size and color. There is a slight asymmetry in the outer halo, but whether this is genuine, or is due to noise, is unclear.
