The galaxy presents as a flattened, elongated structure. A prominent central bulge is visible, exhibiting a yellowish-white hue indicative of an older stellar population. Extending outward from the bulge are faint, diffuse arms with bluer regions, suggesting ongoing star formation. The galaxy appears to be nearly edge-on from our viewing angle, evidenced by the high ellipticity, which obscures any potential spiral structure within the disk. The dust lane may be present within the disk. 

The central bulge is quite large in comparison to the disk and is quite luminous.
