The galaxy presents a roughly elliptical morphology with a smooth, centrally concentrated light profile. The core exhibits a yellowish hue, suggesting an older stellar population or significant dust obscuration. A fainter, bluer halo surrounds the core, extending outwards with a slightly flattened shape. This outer region displays no distinct spiral arm structures or features, and transitions gradually in color and luminosity. The lack of discernible substructure indicates a relatively undisturbed system.
