The galaxy presents as a centrally concentrated elliptical system. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. Moving outward from the center, the galaxy's light gradually diminishes and becomes slightly bluer, hinting at the presence of some younger stars in the outer regions, though the overall stellar population remains relatively old. The galaxy has a smooth, relatively featureless appearance, lacking any distinct spiral arms or significant dust lanes. There are no obvious signs of any major ongoing merger events, or significant tidal disturbances. The general morphology is consistently elliptical in shape.
