This galaxy exhibits a disturbed morphology, appearing to be in a state of interaction or merger. Two primary luminous regions are distinguishable, potentially representing the cores of the merging galaxies. A faint tidal feature or bridge of stellar material seems to connect the two regions, suggesting ongoing gravitational interaction. The overall color is primarily blueish-white, indicating a population of relatively young, hot stars. There appears to be no distinct spiral arm structure visible, potentially disrupted by the interaction. The central regions are brighter, with the light fading at the galaxy's edge. The system is slightly elongated in shape, but the nature of the interaction is difficult to definitively determine without a spectrum.
