The galaxy presents as a smooth, elliptical form, with a high degree of central concentration indicated by the bright, relatively small core. The isophotes appear generally regular. The light profile appears to fade gradually from the core outward, without any clear spiral arms or distinct features. There is a noticeable colour gradient, with the central region appearing more yellow-white and the outer regions exhibiting a slight bluish tint. This colour variation could indicate differing stellar populations or dust content between the inner and outer parts of the galaxy. There's a slight elongation visible, suggesting the galaxy is not perfectly spherical. No prominent dust lanes or tidal features are immediately apparent, suggesting a quiescent state. Based on these observations, the galaxy is likely an elliptical galaxy undergoing minimal current star formation.
