The galaxy appears to be a complex system, possibly in the late stages of a merger event. Two primary concentrations of light are observed, indicating two distinct galactic nuclei or highly concentrated star-forming regions. One of the nuclei has an elliptical appearance and yellow-orange color, indicative of an older stellar population. The second nucleus shows the same features as the first but with a more diffused appearance and an elliptical shape. There is a faint tidal stream or bridge of stellar material connecting the two main bodies, which is blueish, suggesting ongoing star formation. Overall, the galaxy exhibits signs of disturbance.
