The galaxy presents as a merging system, showing significant morphological disturbance. The overall shape is elongated, but dominated by what appears to be 3 distinct large luminous components aligned in a diagonal arrangement. These components are yellow in color. This color suggests a population of older stars. There are no apparent spiral arm features, which is consistent with a likely spheroid or elliptical structure undergoing a merger. Faint extensions emanate from the primary components indicating tidal features and gravitational interaction between the merging bodies. The system lacks significant blue emission indicating low star formation.
