The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellow-white color, indicative of an older stellar population. There is a slight asymmetry in the outer regions, possibly suggestive of a minor gravitational interaction or disturbance. While primarily smooth in appearance, there's a hint of a faint, diffuse disk structure surrounding the core. The galaxy appears relatively isolated with no obvious signs of a major ongoing merger, though subtle disturbances cannot be ruled out. The overall color gradient suggests ongoing, but potentially low, levels of star formation.
