The galaxy presents as a somewhat elliptical and smooth structure. Its overall color profile suggests a more mature stellar population, with a yellowish-white central bulge that may indicate a concentration of older stars. A gradual decrease in intensity from the center outwards is observed, with faint extended areas. No prominent dust lanes or spiral arm structures are discernible; however, there is a subtle hint of asymmetry or possible disturbance in the outer regions. The absence of distinct blue regions implies that the rate of ongoing star formation is relatively low. The overall appearance suggests a relatively massive and evolved galaxy.
