The galaxy presents as a flattened, disk-like structure with a bright, concentrated central bulge. A faint, extended halo surrounds the core, exhibiting a smoother, less structured appearance in the blue/green wavelengths. The central region displays a layered structure, transitioning from a bright yellow/white core to concentric bands of red and blue. The observed colors indicate potential variations in stellar populations and dust content. No significant spiral arm structures are readily apparent, suggesting a lenticular morphology. Minor disturbances may be present given the slight asymmetry in the outer disk.
