This galaxy exhibits characteristics suggesting a possible interaction or merger event. The system appears to consist of two distinct luminous regions with irregular shapes, potentially representing the cores of two galaxies in close proximity. The luminosity profiles of both regions peak sharply, then fade significantly at the outer edges. There is a discernible tidal disturbance or distortion present within the overall structure, characterized by diffuse and asymmetric extensions of light extending outwards. The system's overall color appears blue-shifted, indicating a substantial population of young, hot stars, which could have been formed due to triggered star formation during the interaction. The system displays slight asymmetry and morphological irregularity.
