The galaxy presents as a disrupted spiral structure, exhibiting evidence of a recent or ongoing merger event. There is evidence of tidal disruption visible, with faint tails or streams of stellar material extending outward from the main body of the galaxy, indicative of gravitational interactions with another galaxy. The disk of the galaxy is ill-defined, with regions of patchy star formation and dust lanes scattered throughout. A central bulge is present, but not particularly dominant. There is a relatively high degree of asymmetry observed, with one side of the galaxy showing more pronounced tidal features. The color distribution suggests a mix of stellar populations, with bluer regions likely representing younger stars formed during the interaction and redder regions indicating older, more evolved stars. Based on the disturbed morphology and ongoing merger process, the galaxy is most likely undergoing a period of enhanced star formation.
