The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color appears yellowish-white, suggesting an older stellar population. The central bulge is prominent and significantly brighter than the surrounding regions, indicating a high concentration of stars in the core. There is minimal evidence of spiral arms or significant dust lanes. The outer regions fade gradually, lacking any sharp boundaries or distinct features. The apparent roundness indicates a minimal inclination relative to our line of sight. There are only slight hints of disturbances or interactions with other galaxies. The system exhibits a high degree of symmetry.
