This galaxy exhibits an elliptical morphology with a relatively smooth light distribution, although slight irregularities are visible. The central region appears significantly brighter and bluer than the outer regions, indicating a concentration of younger, hotter stars or active galactic nuclei activity. The outer regions display a faint, diffuse halo. There are some subtle, irregular features that hint at potential past interactions or mergers. The overall color suggests a mix of stellar populations, with a dominant blue component in the core potentially transitioning to a redder hue in the outer regions. Evidence for dust lanes is not immediately apparent.
