The galaxy exhibits an irregular morphology, suggestive of an ongoing or recent merger event. Two distinct, bright central regions are observed, indicative of the nuclei of the merging galaxies. These regions are diffuse, with a yellow-red hue, potentially indicating an older stellar population or significant dust obscuration. There is evidence of tidal features and distortions extending outward, though the relatively faint signal makes detailed characterization difficult. The galaxy's overall shape is somewhat elongated. A faint blue halo surrounds the galaxy.
