This galaxy presents as a generally smooth, elliptical-like structure with a bright, concentrated central bulge. The main body of the galaxy exhibits a relatively uniform color, with subtle gradients suggesting variations in stellar population and dust content. The outer regions appear slightly more diffuse, gradually fading into the background. There is a very slight hint of disk-like structure, but not a definitive disk galaxy. No strong signs of ongoing major mergers or tidal disturbances are immediately apparent, though subtle irregularities might suggest minor interactions. The overall color profile indicates the presence of older stellar populations, potentially with suppressed star formation. It's somewhat intermediate in shape between round and elongated.
