The galaxy presents a primarily smooth morphology with a slight elongation. It appears to be an elliptical galaxy, showing a concentrated central bulge with a gradual decrease in luminosity towards its periphery. There is a hint of a disk, although it is not well defined. The galaxy exhibits a color gradient, transitioning from a yellowish core to a slightly bluer outer halo. No significant signs of recent or ongoing major merger activity are apparent, although a minor disturbance cannot be ruled out. The galaxy's stellar population appears relatively old, with only a small amount of recent star formation activity.
