The galaxy appears to be a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated luminosity, indicative of a significant stellar population. The galaxy's overall color is slightly redder in the central region, transitioning to a bluer hue towards the outer edges. The morphology suggests a galaxy that is not currently undergoing major mergers or significant disturbances. There is a very faint, but perhaps patchy, outer disk, but otherwise it has limited disk-like features visible.
