The galaxy appears to be a relatively smooth, elliptical structure, exhibiting a high degree of circularity. Its color profile suggests an older stellar population, with a dominant yellowish-orange hue. There is a possibility of a minor interaction or disturbance visible as a smaller, redder object situated close to the galaxy's main body, although it is likely that this companion object is merging with the main galaxy. The overall morphology indicates a system that has largely completed its merger history, displaying a relaxed and evolved state.