The galaxy presents as a flattened, elongated structure with a moderately smooth appearance. Its light is concentrated centrally, with a gradual decrease in intensity towards its outer edges. The morphology suggests a disk-like configuration viewed at an angle, possibly a spiral galaxy seen edge-on or a lenticular galaxy. There is a subtle hint of structural irregularity or minor disturbance, but no strong indication of a recent major merger event. Color gradients appear subtle, with a possible slightly bluer hue in certain regions. The overall color profile indicates a relatively evolved stellar population.
