The object presents as a merging galactic system, likely in the late stages of interaction. Two distinct luminous cores are visible, one significantly brighter and more diffuse than the other. The overall morphology is irregular, with tidal features possibly present but poorly resolved in the image. The color suggests a mix of stellar populations, with a dominant yellowish hue indicative of older stars, although some bluer regions may be present. It is difficult to assess the presence of dust lanes or star formation regions due to the image resolution. The system appears to be actively undergoing gravitational interaction, with significant distortion of the original galactic structures.
