The galaxy presents as a disturbed system, possibly undergoing a merger. There are two apparent nuclei separated by a few kiloparsecs based on size estimates. The morphology suggests ongoing or recent star formation. The overall color is a light blue indicating younger stars are present. Evidence of tidal features or extended diffuse emission is visible. The galaxy appears to be relatively low in mass, based on luminosity. It has a relatively high star formation rate considering its mass. The shape is elongated with a high degree of ellipticity.
