This galaxy presents as a disk-like structure viewed at a near edge-on orientation. There is evidence of a central bulge, appearing as a concentration of light that exhibits a yellowish-white hue, indicative of an older stellar population. Surrounding the bulge, a distinct dust lane bisects the galaxy along its major axis, obscuring light from behind. The color of the dust lane appears dark and somewhat blue, consistent with dust absorption. There is a faint, diffuse halo extending above and below the plane of the galaxy. The overall symmetry suggests that the galaxy is relatively undisturbed, although there is some subtle asymmetry in the outer regions. A plume of material is emanating from the galaxy, suggesting a past or ongoing interaction.
