The object presents as two distinct light sources that appear to be interacting or merging. One component is more diffuse and exhibits a yellow-green hue, indicating the presence of ionized gases and ongoing star formation. The other component displays a more concentrated and reddish-orange color, potentially indicating an older stellar population or significant dust obscuration.

There is some evidence that the system is undergoing tidal disruption, causing a distorted appearance and/or a bridge of material that might be present between the two objects. The presence of a merging companion would explain the irregular morphology and the observed star formation.
