The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. The core region exhibits a bright, yellowish-white hue. The radial color gradient suggests the presence of older stellar populations concentrated towards the center. There is little evidence of spiral arms or prominent dust lanes within the observed wavelengths. The galaxy appears fairly undisturbed, showing no signs of major mergers or tidal interactions. The overall shape is quite round, with a slight elongation.
