The galaxy presents as a relatively smooth, centrally concentrated object with a diffuse, extended halo. The central region exhibits a yellowish-orange hue, possibly indicative of an older stellar population. There is a subtle color gradient from the core outward, with the outer regions appearing slightly bluer, suggesting the presence of a younger stellar population in these areas, though less prominent. The galaxy displays a nearly circular morphology and appears to be relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. The overall structure suggests a likely classification as an elliptical galaxy or potentially a lenticular galaxy viewed at a low inclination angle.
