The galaxy presents as a merging system, with two distinct nuclei exhibiting relatively smooth light distributions. The overall morphology appears rounded, though a slight elongation suggests tidal interaction. The color index implies that the object consists of relatively older stellar populations. Faint, diffuse light surrounds the central region, potentially indicative of tidal debris from the interaction. Based on the appearance of two central nuclei, and the surrounding irregular shape, it is very likely this system is undergoing an active merger.
