The galaxy presents a morphology indicative of an ongoing or recent merger event. Distinct tidal tails emanate from the main galactic body, suggesting gravitational disruption. The primary body exhibits a complex structure with what appear to be disrupted spiral arms. These arms show evidence of active star formation, indicated by their bluer color. A prominent dust lane, while not distinctly apparent, is implied by color gradients. There is an elongation along a specific axis. The color profile transitions from a bluer, star-forming disk to a yellower, more evolved bulge region. There appears to be a bar-like feature across the core. Overall, the galaxy is undergoing significant morphological transformation due to the interaction.
