The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a distinct color gradient, transitioning from a reddish-orange core to a greenish-yellow halo, suggesting variations in stellar populations and/or dust content across the galaxy. The absence of well-defined spiral arms or a prominent disk indicates that the galaxy is likely an early-type galaxy. There is a slight asymmetry in the outer regions. Evidence of possible minor disturbances could indicate recent or ongoing interactions.
