The galaxy exhibits a complex morphology suggestive of an ongoing or recent interaction. There appear to be two distinct nuclei, the brighter and more massive of which appears to be somewhat elongated, potentially indicating a disk-like structure seen at an angle. A fainter nucleus resides nearby and is also somewhat elongated. Tidal features, potentially faint arms or bridges, seem to emanate from the main galaxy, and the overall shape is quite disturbed and irregular. The colors are relatively uniform throughout the galaxy, but the nuclei show a subtle redder tinge as compared to the periphery. There appear to be signs of merging, and the system appears to be in a fairly active state of dynamical evolution.
