The galaxy presents as a well-defined, elliptical structure with a smooth, featureless morphology. It exhibits a concentrated central bulge that emits strongly in the yellow-white wavelengths, suggesting a population of older stars. The outer regions of the galaxy display a bluer hue, indicative of ongoing, but subdued, star formation. There is no apparent dust lane or spiral arm structure discernable. The overall light distribution indicates a relatively quiescent state, without major signs of recent mergers or tidal disturbances. The galaxy's shape appears oblate.
