The galaxy presents a complex morphology, suggestive of an ongoing or recent merger event. The light profile is not smooth; instead, it exhibits multiple distinct nuclei or concentrations of luminosity. There appears to be an overall spheroid shape. There are some disk like features, but they are not well defined. The color distribution is heterogeneous, with regions of redder light possibly indicating older stellar populations or dust obscuration, and regions of bluer light hinting at younger star formation. A tidal tail or bridge feature appears to connect the separate light concentrations.
