This galaxy presents as a relatively smooth, centrally concentrated object. The morphology suggests a likely elliptical classification, showing minimal disk features. The core region appears brighter and more yellow-toned, indicating a population of older stars. A fainter, more diffuse blueish halo surrounds the core, suggesting the presence of a younger, albeit smaller, population of stars within its outer regions, and a moderate level of recent star formation. The galaxy exhibits an overall rounded shape, without any signs of significant tidal disturbances or ongoing major mergers, suggesting a relatively undisturbed evolutionary history. There may be some minor irregularities in the outer halo.
