The galaxy exhibits a complex morphology, possibly undergoing a merger event or strong tidal interaction. One primary component appears relatively compact and bright, with a concentrated central region exhibiting a bluish hue, suggesting active star formation. This core is surrounded by a more diffuse, irregular halo with some filamentary structures. A secondary, elongated component is visible, exhibiting a redder color gradient, potentially indicative of an older stellar population or dust obscuration. This component appears significantly fainter than the primary component. Overall, the system displays significant disturbances, challenging classification into a simple Hubble type. Further investigation is needed to determine the full extent and nature of the interaction and its impact on the star formation history of both components. The overall scale appears to be roughly medium-sized.
