The galaxy presents a disk-like structure, viewed at a slight angle from edge-on. A prominent central bulge is visible, exhibiting a moderate size relative to the overall disk. Faint spiral arm structures appear to emanate from the central region, though they are somewhat ill-defined and lack strong contrast. The galaxy appears to be barred, with a relatively strong bar structure going through the bulge. The overall color is bluish, suggesting the presence of younger stellar populations, though the bulge appears to have some yellowing, which may be caused by dust and older stars. The disk appears relatively smooth, with some indications of minor disturbances or tidal features in the outer regions of the disk. There is no obvious indication of any major interaction or ongoing merger event. The light from the galaxy is somewhat faint, which suggests that it is relatively distant.
