The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears centrally concentrated with a noticeable gradient outwards. The overall color is yellowish-orange, suggesting an older stellar population and reduced ongoing star formation. There is minimal evidence of spiral arms or prominent dust lanes. The object shows a high degree of roundness. Based on the smoothness and lack of disk features, it's unlikely to be undergoing any major merging events, though the possibility of a minor disturbance cannot be ruled out.
