This galaxy exhibits a complex morphology, appearing as an ongoing merger event. The primary galactic body is elongated in shape, suggesting a tidal interaction or distortion from the ongoing merger. The luminous central bulge of the primary galaxy is present, with a smooth profile. It appears as a reddish-orange hue, which may suggest an older stellar population in this region.

There is evidence of a smaller secondary structure close to the primary galaxy, it also appears to be smooth and is less redshifted. This could indicate a late-stage merger event or a dwarf galaxy being tidally disrupted. The overall shape of the galaxy appears slightly distorted, likely due to the gravitational interactions between the merging components. Overall, the galaxy appears to be undergoing a significant dynamical event, influencing its shape and potentially its star formation activity.
