The galaxy appears to be in the process of merging. There are two distinct, bright cores, suggesting two separate galactic nuclei. These nuclei display a yellowish-white hue. A faint, diffuse halo of light surrounds both cores, with a slightly more extended and bluish extension visible on one side, potentially indicating tidal features or ongoing star formation triggered by the interaction. The overall shape of the system is irregular, lacking a clear spiral or elliptical structure. A significant portion of the object is unresolved, potentially due to distance or ongoing gravitational disturbances. The system exhibits signs of significant disruption.
