The galaxy presents as a disk-shaped system viewed nearly edge-on. A prominent central bulge is visible, exhibiting a somewhat spheroidal morphology. Dust lanes are subtly present within the disk, obscuring some of the starlight. There is a relatively smooth light distribution across the disk, with no easily discernible spiral arm structure. The galaxy exhibits a blue hue overall, suggesting the presence of a younger stellar population. There is no sign of recent mergers or tidal disturbances to the overall structure.