The galaxy presents as a largely smooth, elliptical-like structure. The core region appears intensely bright and concentrated. Moving outwards, the light diffuses more gradually. A subtle color gradient is visible, transitioning from a predominantly yellow-white hue in the central bulge to a slightly redder tint in the outer regions of the galaxy. There are no prominent spiral arms or dust lanes discernible. The overall shape is generally rounded. There is no clear visual evidence of any ongoing major merger events or significant tidal disturbances affecting the galaxy's morphology, nor obvious signs of active star formation.
