The galaxy presents as a centrally concentrated, smooth object with a slight elongation. The core exhibits a brighter, yellowish hue, which fades into a more diffuse, less luminous outer region that appears slightly bluer. There is no strong evidence of spiral arms or significant dust lanes. Overall, the morphology suggests an elliptical galaxy with a relatively quiescent star formation rate and substantial mass. There are no signs of major mergers or tidal disturbances, although minor disturbances cannot be ruled out at this resolution.
