The galaxy exhibits a moderate level of detail given its apparent size. It appears to be a spiral galaxy undergoing some form of interaction or disturbance. Faint spiral arms are visible, exhibiting a patchy, flocculent structure instead of smooth, well-defined arms. There are possible signs of tidal features or distortions in the overall shape, indicating a gravitational interaction with another galaxy or recent merger event. Distinct regions of star formation or areas of blue, indicative of younger stars are visible. There may be regions of dust obscuration or regions with more red light suggesting older populations. Based on the asymmetry, it is more likely this system is undergoing a merger or tidal interaction with a companion.
