The galaxy presents as a disk galaxy, observed nearly edge-on. A prominent dust lane obscures the midplane, bisecting the galaxy's luminous profile. The bulge component appears smooth and centrally concentrated, exhibiting a near-spherical morphology. Faint extensions suggest possible tidal features or a diffuse halo component surrounding the main disk. The overall color indices indicate a relatively evolved stellar population. The absence of distinct spiral arm features further supports the classification of this galaxy being a relatively evolved system.