The galaxy presents a distorted, asymmetric morphology. It appears to be in the process of undergoing a significant interaction or merger event. A prominent tidal tail extends outwards from the main body of the galaxy in a northeast direction, displaying a distinct blue hue, suggestive of recent star formation. The central region of the galaxy exhibits a somewhat smoother profile with more yellow, indicating the presence of older stellar populations. Multiple distinct clumps or knots of bluish light are observed scattered throughout the galaxy, likely regions of active star formation. There's a region that extends from the center that is more irregular than the central region. There are other smaller regions of higher density of yellow light further along the tidal tail. Based on the morphology, there is significant disturbance.
