The galaxy appears to be in a late-stage merger. Two distinct nuclei, both appearing largely spheroidal and concentrated, are readily apparent. These nuclei are connected by a faint bridge of stellar material. The overall shape of the system is significantly disturbed, with faint tidal features suggesting extensive gravitational interaction and mass exchange. The light distribution indicates an evolved stellar population, with a predominantly reddish-yellow hue throughout the galaxy. The merging process is severely disrupting any pre-existing disk-like structure. There is limited evidence of ongoing star formation. The galaxy is relatively smooth in appearance.
