This galaxy appears to be in the process of a merger. There are two distinct clumps of light, suggesting at least two galactic nuclei. The overall shape is elongated and irregular. There is evidence of tidal tails or bridges connecting the two nuclei, indicated by faint, diffuse emission extending between them. The colors suggest a mix of stellar populations; there is a yellow/orange hue, and possibly some regions of bluer light, indicating star formation. The morphology is disturbed, suggesting a non-equilibrium state likely caused by gravitational interaction. The system appears to be relatively compact, indicating that the merger is likely in its later stages.
