The galaxy presents a largely smooth and rounded morphology. It exhibits a concentrated, luminous core, transitioning into a more diffuse halo. The color profile suggests an older stellar population, with a dominant yellowish-orange hue in the central region. The outer regions appear slightly bluer than the core, though the overall color is more indicative of a relatively quiescent galaxy with minimal current star formation. There is no apparent spiral structure or significant tidal disturbance. There is no clear evidence of mergers or major interactions with other galaxies.
