This galaxy exhibits a smooth, elliptical morphology. The central bulge appears dominant and displays a yellow-orange hue, potentially indicating an older stellar population. There is little evidence of spiral arms or significant dust lanes. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or major mergers in progress, though a slight asymmetry could suggest a minor past interaction. The galaxy is moderately luminous, showing a diffuse and somewhat elongated shape. Overall, it appears to be a fairly evolved system with limited ongoing star formation.
