The galaxy presents as a centrally concentrated, roughly elliptical object with a dominant, bright nucleus. The core region exhibits a yellowish-white hue, suggesting a population of older stars. A fainter, more diffuse halo surrounds the central region. The halo appears relatively smooth, with a gradual decrease in luminosity moving outward from the core. There are some areas that are less concentrated than others, suggesting possible galaxy mergers in its history. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape. There are no apparent spiral arms or prominent dust lanes visible in this image.
