The galaxy presents as a relatively smooth, elliptical morphology, with a high degree of central concentration.  The core exhibits a bright, yellowish-white luminosity, indicating a population of older stars. There's a subtle falloff in light intensity moving outward from the center. The outer regions show a gradual transition to a fainter, more diffuse halo. The overall color is consistent with an evolved stellar population. There is no evidence of spiral arms or active star formation regions. The galaxy appears undisturbed, exhibiting no signs of tidal interactions or recent mergers. Its shape is approximately round.
