The galaxy presents a morphology consistent with a merger event, exhibiting significant tidal disturbances. Two distinct galactic nuclei are visible, one with a more concentrated and defined core, suggestive of a more evolved system. The other nucleus displays a more diffuse appearance. There is evidence of a stellar bridge or tidal tail extending from these nuclei, indicating gravitational interaction. The overall color gradient suggests a range of stellar populations, with redder hues associated with older stars and dust, and bluer tinges potentially indicating regions of recent star formation activity stimulated by the merger. The system’s shape deviates significantly from a regular elliptical or spiral, further supporting the ongoing merger scenario.
