The galaxy presents as a moderately luminous object, characterized by a smooth, elliptical morphology. The light distribution appears concentrated towards the center, suggesting a prominent galactic nucleus. The galaxy exhibits a color gradient, with a slightly redder hue towards the central region, potentially indicating an older stellar population or dust obscuration. There are no discernible spiral arms or prominent star-forming regions visible. The overall form is relatively undisturbed, lacking obvious signs of recent major mergers or tidal interactions. The galaxy appears to be a mature system, exhibiting characteristics consistent with a spheroidal galaxy at a considerable distance.
