The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The light profile suggests an older stellar population, particularly in the core, which displays a yellowish-gold hue. There is a subtle indication of a flattened disk-like structure surrounding the core, though the system appears mostly spheroidal. A minor asymmetry is visible in the distribution of light in the surrounding area. It could be interacting with a smaller system that is causing a minor disturbance. Overall, it exhibits characteristics consistent with a relatively quiescent system nearing the end of its star formation.
