The galaxy presents as a relatively elongated, spiral galaxy. Spiral arms appear present, with a moderate winding. A central bulge is visible, though it appears smaller than the disk component of the galaxy. The bulge appears yellow-white in color, while the disk component presents with a bluer hue overall, hinting at active star formation within the disk. There is some indication of a bar-like structure present, although not distinctly prominent. The galaxy's shape doesn't indicate an ongoing major merger, though minor irregularities or disturbances within the galaxy are plausible from this single image alone. The galaxy appears to be oriented close to face-on with the angle to our line of sight, but with a slight tilt.
