The galaxy presents a smooth, elliptical morphology, with a concentrated central bulge. The light profile appears relatively uniform across the galaxy, lacking any distinct spiral arm structures. Color gradients are subtle but present, the central region exhibits a yellow-orange hue, potentially indicative of an older stellar population. The outer regions show bluer tones, suggesting the presence of younger stars, but this is only subtly present. There is no indication of significant dust lanes or active star formation regions. Overall, the galaxy appears relatively undisturbed, lacking any signs of major mergers or tidal interactions. The round shape suggests a dynamically relaxed system.
