The galaxy presents a disturbed morphology, exhibiting clear signs of an ongoing merger event or significant gravitational interaction. There appears to be two main interacting bodies. The primary, larger component exhibits a smoother light profile with a higher concentration of light towards its core, with a likely more evolved stellar population. A smaller, more irregular component is visible, with bluer hues suggesting younger stars are present. The system's overall colour is relatively uniform, suggesting fairly constant star formation rate across the object. The primary component appears elliptical, or spheroid-like in shape. The overall appearance suggests that the system is in the later stages of a merger, with significant tidal disruption and morphological disturbance, suggesting it is in the process of becoming an elliptical galaxy.
