The galaxy presents as an elongated, relatively smooth object with a noticeable dual core or a merging system exhibiting two distinct central concentrations of light. There is a clear presence of tidal features suggesting ongoing or past gravitational interactions. The galaxy exhibits a reddish hue in the core regions, possibly indicating older stellar populations or significant dust obscuration. Fainter, bluer light surrounds the central regions which may suggest more recent star formation in the extended disk. Overall, the galaxy's morphology appears significantly disturbed, likely due to ongoing merger activity.
