The galaxy presents as a single, largely featureless, and relatively smooth object. Its overall shape is somewhere between round and elliptical with only a slight elongation. The central region exhibits a bright, concentrated core that appears yellowish-white in color, suggesting a population of older stars. This core gradually diffuses outward into a more extended halo of light. There is a subtle color gradient within the galaxy, with the outer regions appearing slightly redder than the core, indicating a possible change in stellar populations or dust content. There is little evidence of spiral arm structure, dust lanes, or active star formation regions visible within the galaxy's disk. No major interactions with other galaxies are obvious in the image. The galaxy displays what might be a very slight disturbance from a gravitational interaction or merger event.
