The galaxy presents a complex morphology, seemingly involved in a gravitational interaction. The primary body exhibits a distorted disk structure. A distinct tidal tail is visible, extending away from the main galactic body, indicating gravitational disruption. This tail appears clumpy, suggesting localized regions of star formation. The galaxy's overall color is yellowish, indicating a mixture of stellar populations, with some regions showing bluer hues potentially associated with younger stars within the tidal tail. The galaxy isn't particularly smooth, with many disturbances. It appears to possibly be merging with multiple galaxies due to its many arms.
