The galaxy presents an irregular morphology, indicative of a system undergoing significant gravitational interaction or disturbance. Two distinct luminous regions are apparent, with one appearing brighter and more compact than the other. A faint, diffuse arm-like structure extends between these regions, suggesting tidal interaction or material stripped from one or both components. This structure may indicate a possible ongoing or recent merger event. The colour gradient within the galaxy appears complex, with subtle variations in hue implying variations in stellar populations or dust content across the system. Some of the disturbed galaxy's light is more red than other areas, this is consistent with ongoing star formation occurring in the galaxy, this indicates that at least some of the disturbance is from a recent collision.
