The galaxy presents as a structured system with a prominent central bulge or core exhibiting a bright, relatively smooth appearance. There is evidence of ongoing or recent interaction or merger activity, indicated by the disrupted morphology and irregular distribution of light in the outer regions. Filamentary structures or tidal tails appear to extend from the main body, suggesting gravitational disturbance. The color distribution indicates a mix of stellar populations, with bluer regions potentially associated with younger stars or active star formation and redder areas possibly indicating older stars.
