The galaxy appears as a centrally concentrated, relatively smooth object. It exhibits a generally elliptical morphology, showing a moderate degree of ellipticity. The core region of the galaxy presents a bright, yellowish-white glow that gradually diffuses outwards. This suggests an older stellar population dominating the central regions, potentially an elliptical galaxy or bulge-dominated spiral. A faint blue tinge surrounds the core, possibly indicating the presence of some younger stars within the galaxy, although the overall star formation activity seems subdued. There's no evidence of strong spiral arms or significant tidal disturbances from interactions with other galaxies. The galaxy appears relatively isolated and undisturbed, with a well-defined boundary.
