The galaxy presents as a centrally concentrated, smooth elliptical system. It exhibits a near-spherical morphology with minimal discernible features, such as spiral arms or distinct dust lanes. The central region displays a higher concentration of luminous material, likely indicative of an older stellar population. The color profile is generally redder towards the core, shifting to a slightly bluer hue in the outer regions, suggesting some ongoing, albeit low-level, star formation activity in its outskirts. No signs of major ongoing mergers or significant tidal disturbances are apparent, although there are some possible signs of minor disturbances. Overall, the galaxy appears relatively isolated and undisturbed.
