The object presents as a merging system comprised of two distinct galactic nuclei. The nuclei exhibit a yellowish-white color, suggesting an older stellar population. The overall morphology indicates significant gravitational interaction and disruption. Tidal features are not immediately apparent, however, the system's irregular shape suggests ongoing or recent merger activity. Based on the color indices, the system is likely massive and contains relatively little ongoing star formation. Overall, the system presents a disturbed morphology indicative of an intermediate stage merger between two galaxies with relatively evolved stellar populations.
