The galaxy presents a complex morphology, appearing as a disturbed spiral structure undergoing a merger. The primary galactic body exhibits discernible, albeit loosely wound, spiral arms. These arms suggest a grand design, though the gravitational interaction disrupts their smooth structure. The central bulge is present, but not overly pronounced. The color gradients within the spiral arms indicate ongoing star formation. Some regions show bluer hues indicative of younger stellar populations, while others display redder tones, potentially indicative of older stars or dust obscuration. A faint stellar stream appears to be emanating from the galactic body, which suggests ongoing tidal interactions with another galaxy. There is evidence of a bar feature. Overall, the system appears to be dynamically active, likely in a late stage of a galactic merger.
