The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentration of light toward the center, indicating a prominent bulge. The core appears yellowish-white, which could indicate an older stellar population dominating the central region. Extending outward from the core, a less concentrated, greenish halo is visible. This halo may suggest the presence of some ongoing, though subdued, star formation activity, or a population of younger stars compared to the core. No distinct spiral arms or bar structures are discernible. The overall color is a gradient from a warm center to a cooler surrounding area. The shape seems generally round, with possibly slight ellipticity. There are no apparent signs of major mergers or significant tidal disturbances influencing the galaxy's structure.
