The galaxy presents as a largely elliptical structure with a high degree of central concentration, and the overall form is smooth and relatively featureless. A bright, concentrated core is evident, suggesting a significant population of older stars. The galaxy exhibits a slight deviation from perfect circularity. Color gradients are visible, with the central regions displaying a yellowish hue, indicating an older stellar population. The outer regions appear dimmer and somewhat redder. There's no obvious dust lane or spiral arm structure visible. The overall appearance is indicative of an early-type galaxy, likely an elliptical or lenticular type. There are no visible signs of major mergers or tidal disturbances. The galaxy appears relatively isolated and relaxed in its morphology.
