This galaxy exhibits a disturbed morphology, possibly undergoing a significant merger event. It presents an elongated structure, suggestive of tidal forces at play. The core region appears relatively smooth and condensed, indicating an older stellar population, while fainter, diffuse light extends outwards. The color profile suggests a mix of stellar populations, with redder hues potentially indicating dust obscuration or older stars. Star formation activity appears to be localized, perhaps triggered by the ongoing interaction. Overall, the galaxy's appearance points to a dynamic system with a complex history of interactions and star formation.
