The galaxy presents as a somewhat edge-on spiral, elongated along its major axis. A prominent central bulge dominates the galaxy's morphology, exhibiting a bright, concentrated luminosity. The disk component appears relatively smooth, lacking significant, easily discernible spiral arm structure. The light distribution suggests a higher concentration of older stellar populations within the bulge. A distinct dust lane or obscuring material is not readily apparent in this image, though some unevenness in the light distribution along the disk hints at possible internal structure. The galaxy exhibits a generally smooth, elliptical light profile.