The object presents as a single galaxy undergoing a major merger. The system exhibits a disturbed morphology, with significant tidal features suggesting strong gravitational interaction. The primary body displays a concentrated, bright core, surrounded by a more diffuse and asymmetrical halo. There is evidence of at least two distinct nuclei or high-density regions within the main structure, implying that at least two galaxies are in the process of merging. One of these appears as an oblong area of light with an orange hue. The tidal tails are faint, but they extend in a sweeping pattern, indicating that the interaction is relatively advanced. The overall color gradient suggests a mix of stellar populations, with the inner regions potentially harboring older, redder stars, and the outer regions possibly hosting younger, bluer stars formed during the interaction. There may be some indications of star forming regions, but more data are needed to determine the exact composition of the galaxy. The shape is irregularly round with little symmetry. 
