The galaxy presents a complex morphology, suggesting a system that is either undergoing or has recently undergone a merger event. A dominant, relatively smooth central component is visible. This component exhibits a slightly elliptical shape. There are at least two fainter features or structures visible in proximity to the primary component. The color of the central component tends towards yellow-white hues, suggestive of an older stellar population, though the presence of bluer knots indicates ongoing star formation. The overall structure is disturbed, further supporting the inference of an interaction or merger. A faint tidal feature can be distinguished between the two main components.
