The galaxy appears as a single, luminous object with a somewhat disturbed morphology, likely a product of an ongoing or recent merger event. Two distinct, bright regions are visible, suggesting the presence of two galactic cores in the process of coalescing. The overall color is yellowish, indicative of an older stellar population, but regions of bluer light suggest more recent star formation is occurring, especially around the brighter core. The galaxy does not appear highly ordered, lacking a clear spiral structure or well-defined disk. The edges of the galaxy appear indistinct, and have minor disturbance in the outer structure, likely due to gravitational interaction. The image suggests that this system is in a state of flux, transitioning towards a more relaxed and potentially elliptical morphology in the future.
