The galaxy appears to be a large, luminous system, approximately 3.3 kpc in radius, at a redshift of roughly 0.109. Morphologically, it seems to be an elliptical galaxy. Its core is relatively smooth and well-defined, with a high degree of roundness. Evident are signs of an ongoing or recent interaction or merger, with what appears to be tidal tail features extending away from the main body of the galaxy. The galaxy shows no apparent features of significant star formation. This indicates it is likely a passive system with a low specific star formation rate.
