The object presents as a merging system or a galaxy with significant tidal disturbances. There is a central concentration of light, but it is irregular and appears to be composed of multiple distinct luminous components. The overall morphology is neither clearly spiral nor elliptical, and exhibits significant deviations from a smooth, regular structure. The system displays a mixture of colors, with some regions appearing bluer and others more red. This suggests a mix of stellar populations, possibly indicating ongoing star formation in some regions and older populations in others. There is evidence of significant interaction or recent merger activity, evidenced by the disrupted morphology and the multiple, distinct luminosity peaks. The structure appears dominated by intermediate-roundness features, trending slightly more towards round than elongated shapes. The colours, overall disrupted morphology, and multi-component structure point to a complex system potentially undergoing a significant evolutionary event.
