The galaxy presents as a merging system. There are two primary, relatively symmetrical concentrations of light, with an elongated, seemingly disrupted morphology suggesting gravitational interaction. The color profile of the main bodies appears somewhat redder, potentially indicating older stellar populations. There is evidence of tidal distortions, and a luminous bridge, or tidal stream, appears to connect the two main components, though this is not very clear. The overall morphology is complex. The galaxy is estimated to have a significant stellar mass and moderate ongoing star formation. The overall structure suggests a late-stage merger event.
