The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-red, suggesting a population of older stars. A diffuse, greenish halo surrounds the bulge. The galaxy's overall shape appears somewhat rounded, lacking any obvious spiral arm structure or bar features, and shows no major signs of ongoing merging activity, though the presence of minor disturbances cannot be entirely ruled out. There does not appear to be much dust or patchiness obscuring the galactic light.
