The galaxy presents as an elliptical-like system, with a smooth, centrally concentrated light profile. The core exhibits a yellowish-white hue, indicative of an older stellar population, potentially dominated by red giants and older main sequence stars. Moving outwards from the core, the color transitions to a bluish-white, suggesting a lower proportion of older stars and possibly ongoing, though moderate, star formation in the outer regions. There are no prominent spiral arms or a clear disk structure visible. The overall shape is somewhat spheroidal, but it is not perfectly circular, with a slight elongation along one axis. There are no clear signs of major disturbances, tidal tails, or other morphological features that would strongly suggest recent mergers or interactions with other galaxies.
