The galaxy exhibits a disturbed morphology, suggesting a potential interaction or merger event. There appears to be a main body alongside a secondary, less-defined component. A tidal tail is visible on one end. The color distribution is uneven, with patches of blue indicating regions of ongoing star formation and reddened areas potentially indicating older stellar populations or dust obscuration. The overall shape is moderately elongated. The system shows evidence of internal disruptions, possibly due to gravitational interactions.
