The galaxy presents a generally smooth morphology, exhibiting a dominant, spheroidal structure. The color profile indicates a concentration of older stellar populations, with a yellowish-orange hue dominating the central region. There's a slight elongation noticeable, moving away from the round, more towards a football shape, but not greatly so. No distinct spiral arms or prominent dust lanes are visible within this image, supporting the observation of a relatively smooth galaxy. There is no signs of tidal tails, or shells of stars, so no significant mergers appear to be taking place.
