The galaxy presents a flattened, disk-like morphology, with a notable bulge at its center. The orientation suggests it is viewed at an oblique angle, somewhere between face-on and edge-on. The central bulge exhibits a yellow-white hue, indicative of an older stellar population. Extending outward from the bulge is a fainter, bluer disk, suggesting the presence of younger stars and ongoing star formation. The disk is not perfectly uniform; subtle variations in color and brightness hint at spiral arm structures, although these are not sharply defined. The galaxy's light profile appears relatively smooth, with a gradual decrease in surface brightness from the center to the outer regions. Some dust is present, subtly reddening the color of the disk.
