The galaxy presents as a system of interacting galaxies or a galaxy undergoing a major merger. There are at least two distinct nuclei visible, suggesting multiple progenitors. The system exhibits a disturbed morphology, lacking a clear, defined spiral or elliptical structure. The color profile suggests a complex mix of stellar populations. Some regions appear bluer, possibly indicative of ongoing star formation. Other regions are redder, perhaps indicating older stellar populations. There is no clear evidence of a prominent disk structure, although the presence of tidal tails or bridges of material connecting the galaxy suggests the possibility of a disk system being distorted due to the interaction. The spatial extent is moderate, neither highly compact nor vastly spread out. The overall appearance indicates a dynamically active system, likely evolving significantly due to the gravitational interactions between its components.

