The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, condensed appearance, transitioning to a fainter, more diffuse outer region. Color gradients are subtle, with a slightly bluer hue in the central region suggesting the presence of younger stellar populations, while the outer regions appear redder, consistent with older stars. There is no evident spiral structure or distinct disk component. No signs of tidal disturbances or recent merger activity are apparent from this imagery.
