The galaxy presents as a concentrated, elliptical structure. The central region exhibits a bright, yellowish-white hue, indicative of a substantial population of older stars. Progressing outward from the core, the light gradually diffuses, transitioning to a less concentrated, fainter halo. The axial ratio suggests a moderate degree of flattening, with the galaxy appearing elongated along a defined axis. There is no apparent spiral structure or active star formation regions visible in the image. A smooth, relatively featureless morphology is observed, suggesting a more evolved system with minimal ongoing interactions or mergers.
