The object appears to be a spiral galaxy undergoing a significant merger event. Evident are morphological disturbances indicative of a major interaction. The main body shows complex, irregular features, with a suggestion of distorted spiral arm structures extending outward from the central region. The luminosity distribution suggests a substantial population of young stars, implied by the galaxy's moderate star-formation rate. While the galaxy is undergoing a merger, one of the merging galaxies is likely a larger galaxy with an apparent disk. The overall color profile indicates a mix of stellar populations, consistent with ongoing star formation and older stellar components within the bulge and disk. There is no clear bar structure.
