The galaxy presents a largely spheroidal morphology, exhibiting a smooth, concentrated central bulge. There is little discernible structure in the form of spiral arms or a prominent disk. The color appears yellowish-red, suggesting an older stellar population and a relative lack of ongoing star formation. The outer regions fade smoothly into the background, indicating a gradual decrease in stellar density away from the core. The galaxy appears relatively undisturbed, lacking any obvious signs of recent mergers or tidal interactions. Its overall appearance suggests a mature, passively evolving system.