The galaxy presents a flattened, disk-like morphology indicative of a spiral structure. Two well-defined spiral arms emanate from a central bulge region. These arms appear relatively tightly wound, with a medium pitch angle. The color distribution suggests active star formation along the spiral arms, evidenced by bluer hues. A central bulge is present, appearing moderately sized. There is no major disturbance or significant evidence of a recent major merger event, though minor irregularities may indicate some ongoing interaction or accretion. The galaxy does not appear to be viewed edge-on, but rather at a slight angle that allows the spiral structure to be clearly discerned.
