This galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction. Two distinct luminous components are observed, potentially representing the cores of two galaxies in the process of merging. A tidal bridge-like structure appears to connect the two components, indicating gravitational interaction and mass transfer. The overall shape is elongated and irregular, deviating significantly from a typical elliptical or spiral form. The light distribution seems fairly smooth, but there are possible faint blue regions suggesting active star formation.
