The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. Its color profile exhibits a dominant yellowish hue, suggesting an older stellar population with reduced ongoing star formation. There appears to be a slight asymmetry or minor disturbance in the galaxy's structure which could possibly suggest a minor gravitational interaction or merger event. The main body of the galaxy is relatively compact. Overall, this galaxy appears to be a fairly quiescent system.
