The galaxy appears to be an interacting system comprised of two distinct luminous components. The brighter, upper component exhibits a generally smooth morphology. The lower component is less bright. Both components present a blue-ish hue, potentially indicative of ongoing star formation activity. The overall morphology is disturbed and elongated. The system appears to be in the midst of a tidal interaction, with potential tidal tails or debris. The overall shape seems closer to elliptical than spiral.
