The galaxy presents as a disturbed system, quite possibly undergoing a merger. Two distinct, bright concentrations of light are apparent, suggesting either two galactic nuclei or a single nucleus and a significant area of intense star formation. The overall morphology is elongated and irregular, lacking a well-defined disk or spiral structure. The light emitted is relatively red, indicating a population dominated by older stars. There appear to be significant tidal features or disturbances around the main body of the galaxy. The galaxy appears to be relatively massive. Current star formation is happening at a moderate rate.
