The galaxy presents a relatively smooth, elliptical morphology with a high degree of central concentration. Its apparent color index suggests a population of older stars, with a dominant yellowish-red hue. There is some evidence of a fainter, bluer halo surrounding the central region, which may indicate a small amount of ongoing star formation. The galaxy's roundness indicates that it is likely viewed close to face-on. The overall appearance is relatively undisturbed, with no clear signs of major merging events or significant tidal distortions.
