The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core region exhibits a yellowish-white hue, which could indicate a population of older stars and reduced active star formation within that region. The galaxy's overall shape is mostly round. Faint blue regions in the outer parts of the galaxy suggest there might be limited areas of ongoing star formation or younger stellar populations present. The galaxy appears to be undisturbed, lacking any obvious signs of recent or ongoing major mergers or tidal interactions.
