The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The central region exhibits a yellowish-orange hue, potentially indicating an older stellar population. A subtle greenish halo surrounds the core, which could indicate the presence of younger stars or ionized gas, though the overall color profile suggests relatively low star formation activity. The galaxy appears moderately luminous and relatively undisturbed, without any obvious signs of tidal features or ongoing mergers. It displays a predominantly smooth structure, with only the slightest suggestion of any disk-like features. The galaxy shows an intermediate ellipticity.
