The galaxy presents a complex morphology suggestive of an ongoing or recent merger event. Two distinct, bright nuclei are visible, indicating the likely presence of two separate galactic cores interacting. A diffuse, extended halo of stellar material surrounds the nuclei, exhibiting an irregular shape that deviates from a typical elliptical or spiral structure. This halo displays a smooth texture, although it is not uniformly distributed. There is a general reddish-orange color, indicating that the galaxy likely hosts an older stellar population, though some bluer regions are present, possibly indicating ongoing or recent star formation. There is evidence of tidal features, such as faint stellar streams or bridges extending outwards from the main body of the galaxy, hinting at the gravitational disruption caused by the interaction.