The galaxy presents as a smooth, elliptical form, with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, suggesting a significant population of older stars. Progressing outward from the core, the intensity of light gradually diminishes. The outer regions display a subtle reddish tint. A slight elongation is observable, hinting that the galaxy is not perfectly spherical, but rather has a cigar-like shape. There is no clear evidence of spiral arms or dust lanes. No signs of any major merging events or strong gravitational disturbances are apparent. Overall, the galaxy seems to be in a relatively quiescent state.