The galaxy presents as a centrally concentrated, elliptical morphology. The core exhibits a yellow-white hue, indicative of a population of older stars. There is a gradual decrease in surface brightness moving outwards from the nucleus. The outer regions appear more diffuse and slightly redder in color than the core, perhaps suggestive of dust absorption or a population shift towards redder stars in the outskirts. No prominent spiral arms, bars, or distinct features are discernible. The overall structure appears relatively smooth and undisturbed, with no obvious signs of tidal interactions or ongoing mergers. The galaxy's color profile suggests an evolved stellar population and a low rate of recent star formation.
