The galaxy appears to be undergoing a significant interaction, potentially a merger. There are two distinct, bright cores visible. One core exhibits a yellow-white hue, possibly indicating an older stellar population. The second core presents a redder color, suggesting ongoing star formation or significant dust obscuration. The overall shape is irregular, lacking a clear spiral or elliptical structure. Diffuse light surrounds the two cores, extending outwards in an amorphous halo. Evidence of tidal tails or bridges of material is subtle, but hints of disturbed structure are present in the outer regions of the galaxy. The system demonstrates a moderate redshift, positioning it at a considerable cosmological distance. The observed color indices imply a moderate to high luminosity. The morphology suggests a recent or ongoing dynamical event, possibly triggered by a merger between two galaxies of substantial mass.
