The galaxy presents a complex morphology, appearing as a system undergoing a significant interaction or disturbance. Its overall structure suggests a generally smooth central component, but it is distorted by features indicative of ongoing gravitational interactions.

There are two distinct bright regions within the galaxy, potentially representing the original cores of merging galaxies or bright star forming regions stimulated by the ongoing interaction. A faint tidal feature emanates from the central region, suggestive of material being stripped away from the main body of the galaxy due to gravitational forces. These features indicate active dynamics and possibly recent or ongoing star formation activity within the system. The color distribution suggests some variation in stellar populations or dust content across the galaxy.

