The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction. There is a clear indication of a possible merger event. The galaxy's light profile appears asymmetrical, and there is evidence of tidal features or distorted arms extending from the main body. A significant portion of the galaxy's light is concentrated in a central region, potentially indicating a bulge. The color gradient suggests a mix of stellar populations, with the bluer regions potentially indicating ongoing star formation. The presence of multiple luminous knots or clumps within the galaxy may represent star-forming regions or the remnants of the merging components. Overall, the galaxy appears to be in a dynamically active state.
