The galaxy presents as a flattened, disk-like structure, oriented nearly edge-on with respect to our line of sight. A prominent central bulge appears smoothly concentrated and somewhat spheroidal in shape. The bulge exhibits a yellowish color, suggesting an older stellar population. The disk component appears considerably fainter and more diffuse, with a subtle gradient in brightness outward from the central bulge. The color profile of the disk appears somewhat bluer than the bulge, potentially indicating the presence of younger stars and ongoing star formation. There appears to be only slight asymmetries or distortions visible in the overall structure.
