The galaxy presents a disturbed morphology, possibly indicative of a merger event. Two distinct nuclei are observed. The nucleus located to the western side is primarily yellow in color, suggesting an older stellar population or significant dust obscuration. In contrast, the eastern nucleus is notably redder, potentially indicating a distinct stellar population or a region of intense star formation obscured by dust. The overall shape is somewhat elongated, with evidence of tidal tails or disrupted spiral arms extending from the main body. There is some smoothness within the central area which could represent the remnant of a disk but is likely disturbed. The low surface brightness of the surrounding regions suggests it is older with a low star formation rate.
