The galaxy presents as an elongated, edge-on spiral system. A distinct central bulge is visible, exhibiting a yellowish-white hue, suggesting a population of older stars. Extending outwards from the bulge along the major axis is a disk component, exhibiting a bluer coloration. This indicates the presence of younger, hotter stars and ongoing star formation. Dust lanes may be obscuring some of the light from the disk, creating a somewhat patchy appearance in the bluer regions. The disk appears relatively thin and well-defined. There is a suggestion of faint tidal features or minor disturbances, but the overall morphology suggests a relatively undisturbed system.
