The galaxy presents as a central, bright, relatively smooth bulge. The color of the central region suggests active star formation or a potential active galactic nucleus, as indicated by the green hue. Extending from one side of the central bulge is a fainter, elongated structure. The color shifts in this extension, transitioning from blue to red, suggesting varying stellar populations and/or dust extinction along the structure. The overall morphology suggests the possibility of a tidal tail resulting from a past interaction or merger event, though the central region retains a largely undisturbed appearance. A minor asymmetry is apparent in the bulge.
