The galaxy presents an elliptical morphology, exhibiting a smooth and concentrated light profile. Its color index suggests a population of older stars, with a dominant yellowish hue at the core. While largely smooth, a faint hint of structure is observed. The galaxy appears relatively undisturbed, with no evident signs of major mergers or tidal interactions. The lack of prominent blue regions indicates a low rate of ongoing star formation. Overall, the galaxy appears to be a mature, passively evolving system.
