The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a yellow-orange hue, suggesting a population of older stars and a relatively low rate of current star formation. The light is concentrated in the center, with a gradual decrease in surface brightness towards the outer regions. There is no evidence of spiral arms or a prominent disk structure. The galaxy appears largely undisturbed, with no significant signs of tidal interactions or major mergers. The general shape is slightly elongated, but not extremely so.
