The galaxy exhibits a disturbed morphology, indicative of a possible ongoing or recent interaction. Evident are some features indicative of possible tidal tails or disrupted arms extending from the central region. The light distribution appears uneven, with brighter concentrations and fainter, diffuse areas scattered throughout the body of the galaxy. There is some hint of a disk component, but the prominence is low. The core region appears somewhat condensed. The galaxy appears to be relatively faint, and potentially has a low star formation rate. There is also a possible merging event occurring.
