The galaxy presents a complex morphology suggestive of an ongoing or recent interaction. The primary body of the galaxy exhibits a flattened, elongated shape. There is a secondary, more compact component situated nearby, potentially indicating a close companion or a nucleus undergoing a merging process. The overall color profile appears to be dominated by older stellar populations, indicated by the yellowish hues. The system exhibits some signs of minor disturbances in its overall structure. Further analysis would be necessary to determine the precise nature and evolutionary stage of this galactic interaction.
