The galaxy presents as a relatively smooth, elliptical structure with a concentrated core. It exhibits a moderate ellipticity, appearing as a slightly elongated spheroid rather than a perfect circle. The color profile suggests a higher concentration of older stellar populations. There's a subtle asymmetry in its outer regions, possibly indicating a minor gravitational disturbance. The image does not reveal any clear signs of spiral arm structures or significant dust lanes. The galaxy's outer halo gradually fades into the background sky, making it difficult to precisely define its outer boundaries. The light distribution indicates that the galaxy is relatively well-mixed with the majority of stars concentrated at the core.
