The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge. The core is a bright, yellowish-orange hue, suggesting a population of older stars with low levels of ongoing star formation. The outer regions of the galaxy gradually fade into a diffuse halo, exhibiting a slightly bluer tint than the core, possibly indicating the presence of a younger stellar population, though this is minimal. There is no clear evidence of spiral arms or a distinct disk component. The overall morphology implies a relatively evolved system, potentially with a high mass, with only minor, if any, signs of recent mergers or disturbances. The galaxy's shape is close to round, with a slight deviation indicating an in-between shape.
