The galaxy presents as a relatively smooth, centrally concentrated object with a discernible, but not dominant, disk-like structure. The central region displays a bright, yellowish-white core, likely indicating a high concentration of older stellar populations. This bright core fades smoothly into an extended halo with a more diffuse, yellowish-orange hue. The overall morphology leans towards a spheroid, but with a slight elongation that suggests the presence of a flattened component. Subtle irregularities are present in the outer regions of the halo, potentially indicating minor tidal interactions or internal disturbances. There's no strong evidence of prominent spiral arms or significant dust lanes from the available imagery. The color suggests a relatively evolved stellar population, with ongoing but possibly subdued star formation.
