The galaxy presents as a centrally concentrated system with a roughly elliptical morphology. Its core exhibits a bright, unresolved nucleus that gradually fades into a surrounding stellar bulge. The bulge region appears relatively smooth, lacking prominent dust lanes or distinct features. Faint spiral arms can be tentatively discerned, appearing loosely wound and somewhat patchy in their star formation activity. A diffuse, extended halo surrounds the main body of the galaxy, suggesting the presence of a significant stellar population beyond the more concentrated regions. Overall, the galaxy exhibits an intermediate disk component with a mix of older stellar populations. There are some subtle signs of minor gravitational disturbance, such as asymmetries or distortions in the outer regions of the disk.
