The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The color becomes slightly redder towards the outer regions of the galaxy, further supporting this hypothesis. There is no discernible spiral structure or distinct dust lanes visible. Faint blue light is scattered throughout. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or recent mergers. Overall, the galaxy presents as a massive, evolved system likely dominated by an older stellar population.
