The galaxy presents as an early-type spiral galaxy. It exhibits a relatively smooth, oval-shaped morphology with a notable central bulge. Diffuse arms are present, though not sharply defined, indicating a more flocculent spiral structure rather than a grand design spiral. The disk component appears to be viewed at a shallow angle, closer to face-on than edge-on. There's a slight color gradient visible, transitioning from a bluer hue in the outer disk to a somewhat yellower tone toward the galactic center. The absence of prominent dust lanes suggests a lack of significant amounts of interstellar dust within the galaxy. There are no indications of any major ongoing merging activity, though some minor disturbances cannot be ruled out entirely.