The galaxy presents as a smooth, elliptical morphology, with a high degree of central concentration. The light profile appears relatively even across the galaxy, with a slightly elongated shape, more akin to an oval than a perfect sphere. The core region exhibits a warmer color temperature, indicated by the yellowish-orange hue, possibly suggesting an older stellar population and/or dust obscuration. The outer regions of the galaxy transition to a bluer color, hinting at the presence of younger stars or a different stellar population mix in the periphery. There is no obvious evidence of spiral arms, strong dust lanes, or other distinct features typically associated with disk galaxies. No apparent signs of ongoing major mergers or significant tidal disturbances are visible. Overall, the galaxy gives the visual impression of an elliptical galaxy with a relatively quiescent star formation history.
