The galaxy presents as a moderately luminous, elliptical morphology with a smooth, centrally concentrated light profile. The core exhibits a yellowish-white hue, suggesting an older stellar population. A more diffuse, bluish halo surrounds the central bulge, indicating the presence of a younger stellar population and possibly ongoing, albeit low, star formation. The galaxy appears somewhat elongated, and its overall structure seems relatively undisturbed, with no major signs of tidal interactions or recent mergers visible.
