This galaxy appears to be a relatively luminous object at a considerable distance. The light profile suggests a centrally concentrated spheroid, exhibiting a smooth, round morphology. The core region displays a yellowish-orange hue, possibly indicating an older stellar population. There is a subtle extension that seems to be less concentrated, with a bluer tint, potentially suggesting some ongoing star formation in a more diffuse structure. Overall, the galaxy appears to be relatively undisturbed, without any obvious signs of major mergers, although there could be some minor disturbance or interaction influencing the slight asymmetry and faint features in the extension.
