The galaxy presents as a spiral structure with a prominent central bulge. Two clearly defined spiral arms emanate from a central bar feature, exhibiting a tightly wound morphology. A moderate amount of ongoing star formation appears to be occurring throughout the arms, based on a blue tint observed, though the exact rate of star formation requires further spectral analysis. The central bulge appears relatively smooth and concentrated, implying it is a well-established structure within the galaxy. No signs of major disturbance are visible. The disk is not edge-on, suggesting a face-on or nearly face-on orientation relative to the observer.
