The galaxy exhibits a centrally concentrated morphology, appearing largely smooth and elliptical. The light profile indicates a high degree of symmetry. There is an absence of any readily discernable spiral arm structure or pronounced dust lanes. The galaxy is yellowish white, suggesting an older stellar population dominates. The absence of blue light suggests a low rate of on-going star formation. The object seems undisturbed, showing no obvious signs of tidal interactions or ongoing merger activity. The overall appearance suggests a relatively quiescent galaxy, with evolved stellar populations and a smooth overall structure.
