The galaxy presents as a disk-shaped system, viewed at a near edge-on inclination. A prominent central bulge dominates the visual appearance, exhibiting a smooth, bright profile. The bulge appears yellowish-white, suggesting a population of older stars. Fainter, bluer light extends outwards from the bulge, tracing the galactic disk, though any spiral arm structure is indistinct. This outer disk appears relatively smooth. The galaxy shows no signs of strong disturbances or ongoing major mergers. The disk is relatively thick, with a subtle dust lane visible along the central plane, implying the presence of interstellar medium. Star formation is suspected to be present, but relatively low overall, and mostly limited to the disk. The system exhibits moderate mass.
