This galaxy appears to be an interacting system, possibly in the late stages of merging. The overall structure appears complex and disturbed, with potentially three distinct luminous clumps that might represent the cores of the original galaxies. The shape is largely irregular, rather than showing a clear spiral or elliptical morphology. There is a general golden color suggesting an older stellar population, but some bluer tinges in certain areas hint at ongoing, though not necessarily intense, star formation within the system. The system is of moderate size, with some low-surface brightness material surrounding the bright core regions, indicating tidal interactions or remnants of the merging process.
