The galaxy presents as a somewhat elongated, disk-shaped system viewed at an oblique angle. The central bulge region exhibits a bright, concentrated luminosity, appearing primarily yellowish-orange in color, suggesting a population of older stars. Proceeding outward from the core, the disk reveals a broader, fainter distribution of stars and dust. Hints of spiral arm structure are discernible, although they are not sharply defined. There's a blue tint to the galaxy when viewed from the outer-most regions. A faint, diffuse halo is visible, extending beyond the main body of the galaxy. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of major merger events or tidal interactions.
