The galaxy presents a largely smooth, elliptical morphology. It exhibits a central concentration of light that gradually diminishes towards the outer regions. The color profile suggests an older stellar population, as indicated by the redder hues. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There is a subtle hint of a possible disk, but the dominant feature remains its spheroidal shape. Star formation is likely present, but at a low rate, given the overall color and smooth structure. There are no prominent dust lanes or spiral arms visible.
