The galaxy presents a disturbed morphology, appearing to be in a late stage of a major merger. The system displays two distinct, luminous components, likely the remnants of the progenitor galaxies' cores. These cores exhibit a yellowish-orange hue, suggesting an older stellar population or significant dust obscuration. Tidal features, such as faint extended arms or diffuse light, are apparent. These distortions indicate strong gravitational interactions. Overall, the galaxy appears to be a dynamically active system undergoing a significant transformation due to the ongoing merger event, which has likely triggered elevated levels of star formation within the galaxy.
