The galaxy exhibits an irregular morphology, appearing as a system undergoing a significant merger event. There is a prominent, relatively smooth component, possibly a bulge or core of one of the merging galaxies. Evident are tidal features or disturbances, indicating ongoing gravitational interactions. Bright regions of star formation are visible, with distinct color variations suggesting differing stellar populations or dust obscuration within the galaxy. The overall color of the galaxy is a blend of blue and red, hinting at both young, hot stars and older, cooler stellar populations. The shape appears neither fully elliptical nor spiral, but rather distorted, consistent with late-stage merger dynamics.
