The object presents as a disturbed system, suggestive of a galaxy merger in progress. Multiple components are visible, including a brighter, more compact core with what appears to be tidal features or disturbed spiral arms extending outwards. These arms show a mottled texture, potentially indicative of active star formation regions. There is a secondary component that may be another galaxy involved in the interaction. The overall morphology is irregular and asymmetric, lacking a well-defined disk or elliptical shape. The colors suggest a mix of stellar populations, with bluer regions potentially indicating younger stars and ongoing star formation, and redder regions potentially indicating older stellar populations. Overall, the system shows clear evidence of a dynamic interaction and merger event shaping its structure and stellar content.
