The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration.  The luminosity appears relatively uniform, lacking prominent spiral arms or distinct features suggesting ongoing star formation on a large scale. The core region is noticeably brighter and appears slightly elongated, trending towards an intermediate, but not perfectly round, shape. Faint extensions are present, indicating it is not a perfect circle. Subtle color variations are visible, transitioning from a yellow-orange core to a slightly greener outer halo, possibly indicating differing stellar populations. There are no apparent signs of major mergers or significant tidal disturbances, although a possible minor disturbance could be present due to the slight irregularities in the outer regions.
