The galaxy appears to be undergoing a merger or experiencing significant gravitational interaction with at least one other galaxy. The primary body of the galaxy exhibits a generally smooth morphology but with distinct disturbances and asymmetries. There is evidence of tidal features or disrupted structures, suggesting a recent or ongoing interaction. 

The galaxy presents an overall slightly rounded appearance, though not perfectly spherical. The light distribution is somewhat irregular. The color profile suggests a mix of stellar populations, with areas exhibiting bluer light indicative of younger, hotter stars and other regions presenting redder hues, potentially indicating older, cooler stars or dust obscuration. The system is compact, and the merging or interacting components are closely associated. 
