The galaxy presents as a system undergoing a significant merger. The primary body exhibits a largely smooth, elliptical morphology, appearing quite round, but there are clear signs of interaction with two smaller companions. Two prominent yellow-orange clumps of light are visible north of the main body. They appear as separate concentrations of stellar mass, and are connected by faint arcs. The light from these clumps suggests older stellar populations. To the southeast of the main body, there is an elongated region of diffuse light that contains some bluer stars. These features suggest tidal interactions and ongoing star formation induced by the merger event. There is an absence of prominent spiral arm structures within the system. The overall color of the main body appears more redshifted than the merging features, suggesting it's a more evolved, massive component. Dust lanes are not clearly visible, but may be present given the color variations observed. The system is not fully relaxed and demonstrates significant dynamic activity.
