The galaxy presents a complex morphology suggestive of an ongoing or recent merger event. Two distinct, bright nuclei are visible, indicating the presence of two progenitor galaxies interacting. The system appears relatively smooth, yet displays some features indicating disturbances. There is a general roundness to the overall structure. The primary color profile of the galaxy is yellowish, suggesting a population of older stars, but there are pockets of greener hues, which potentially indicate younger stars. The overall system is moderately luminous.
