The galaxy presents as a generally smooth and centrally concentrated object. It exhibits a spheroidal morphology, with a noticeable bulge in the center that transitions into a more diffuse, less luminous halo. There may be a very subtle disk but is hard to be certain. The color profile suggests a mix of stellar populations. The central region displays a yellowish hue, indicative of older, redder stars. The outer regions of the galaxy appear slightly bluer, suggesting the presence of younger, hotter stars, though this population seems less dominant. There is little indication of dust lanes or significant spiral arm structure within the image, supporting the classification as a relatively evolved system. The galaxy appears relatively isolated, with no immediately obvious signs of tidal interactions or merging activity. It seems to be a stable, relatively undisturbed system.
