The observed galaxy presents a morphology suggesting an ongoing or recent merger event. Two distinct, luminous cores are visible, indicating the presence of two galactic nuclei in close proximity. The shapes of these cores are somewhat irregular, deviating from a perfect elliptical or spiral form, which could indicate gravitational disruption. Diffuse, extended emission surrounds the cores, forming a common envelope that links the interacting components. This extended halo has a reddish hue, possibly indicating older stellar populations. Overall, the system appears to be in a dynamic state, with potential tidal features or distortions that cannot be clearly resolved due to the image resolution and distance. Further spectroscopic analysis would be valuable to determine the relative velocities of the components and confirm the merger status.