The galaxy presents as a merging system, displaying two distinct, bright nuclei. The overall morphology appears relatively smooth, with a diffuse, extended halo surrounding the two primary components. There is a hint of a bridge of material connecting the nuclei. No strong dust lanes or spiral arm structures are clearly visible, which could imply that we are observing an early stage merger. The color appears moderately blue, suggesting ongoing star formation. The merging system appears slightly elongated, but with significant roundness, possibly indicative of the interaction process beginning to coalesce into a single object.
