The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. It displays a relatively round shape. The central region is bright and appears yellowish-white, suggesting an older stellar population. The outer regions appear fainter and slightly bluer, potentially indicating some degree of ongoing, low-level star formation or a population of younger stars compared to the core. There is no discernible spiral structure or any evidence of significant tidal disturbances or mergers. The galaxy appears fairly isolated and undisturbed.
