This galaxy exhibits a generally amorphous morphology, with a centrally concentrated luminosity profile suggesting an elliptical or lenticular classification, but displays strong evidence of an ongoing or recent interaction or merger event. The overall color is suggestive of an older stellar population, with a redder hue prominent throughout, though a slight blue component can be detected. Multiple distinct luminous clumps are visible within the central region, suggestive of merging components and star formation. There is a distinct irregularity in the overall shape, deviating from the typical smooth profile seen in undisturbed elliptical galaxies. Hints of faint tidal features are present in the outer regions, although these are not sharply defined. These could indicate the remnants of a past interaction or the initial stages of a continuing merger. The morphology indicates this system is dynamically active, and it may evolve into a more relaxed elliptical galaxy over time.
