The galaxy presents as a largely featureless, smooth elliptical form, exhibiting a notable central bulge with a high degree of spheroidal symmetry. There's a distinct color gradient observed, with the core region appearing more yellow/gold, transitioning to a redder hue in the outer regions of the galaxy. No distinct spiral arms or prominent dust lanes are visible. The galaxy appears relatively isolated with no obvious signs of recent major merger events. Faint tidal features may exist but the image resolution is insufficient to confirm. The overall morphology suggests an evolved system. The general smoothness and color indicate a stellar population dominated by older, redder stars, with a low rate of on-going star formation activity.
