The galaxy presents a morphology suggestive of an ongoing or recent interaction, possibly a merger. The system exhibits a complex structure with two distinct bright, reddish cores or nuclei. These cores are embedded within a more diffuse, greenish-blue halo of light. The general shape is somewhat elongated, trending towards a circular appearance. The redder colors of the core regions may indicate older stellar populations or dust obscuration, while the bluer halo suggests the presence of younger stars and ongoing star formation. There appears to be some structural disturbance or asymmetry in the outer regions, hinting at tidal effects resulting from gravitational interaction.
