The galaxy presents as a smooth, elliptical object with a high degree of central concentration. The core appears bright and yellowish-white in color, suggesting a population of older stars. There is a slight elongation to the galaxy's shape, deviating from perfect circularity. The color becomes subtly redder as the radius increases outward from the core, possibly indicating a change in stellar population or dust content in the outer regions. No distinct spiral arm structures or significant dust lanes are apparent. There are no obvious signs of recent major mergers or tidal disturbances in the galaxy's morphology, such as plumes or extended halos. Overall, this galaxy exhibits the characteristics of a relatively evolved, quiescent system.
