The galaxy presents as a generally smooth, centrally concentrated object. The morphology appears largely elliptical, transitioning from a bright, condensed core outwards to a more diffuse halo. No spiral arm structures or significant dust lanes are discernible within the limits of the image resolution. The light profile demonstrates a smooth gradient, suggesting a relatively evolved stellar population. There is a possible slight asymmetry to the outermost isophotes, but it's difficult to fully discern whether this is a tidal feature or an artifact of the image quality. Overall, the galaxy appears to be an early-type, relatively undisturbed system, likely at a considerable distance.
