The galaxy appears to be a spiral galaxy, viewed edge-on. The central bulge is prominent and appears relatively smooth, with a yellowish hue, suggesting a population of older stars. Dust lanes are faintly visible along the galactic plane, obscuring some of the light from the bulge. The disk of the galaxy is elongated and has a bluer color compared to the bulge, indicating the presence of younger stars and ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. It has a generally smooth appearance. There are faint indications of spiral arm structure extending from the bulge into the disk, although they are not well-defined.
