The galaxy appears to be a relatively smooth, elliptical or lenticular type, exhibiting a high degree of circularity. The light profile suggests a concentrated nucleus that is likely a supermassive black hole. There is some evidence of a faint extended halo surrounding the central region, however no distinct structures, such as spiral arms or a prominent disk, are visible. The overall color of the galaxy is yellowish-orange, suggesting an older stellar population with fewer young, massive stars. There is only very subtle variation in color across the galaxy, which indicates the galaxy is relatively old. The lack of substantial dust lanes or patches supports the hypothesis of an elliptical morphology. The galaxy appears isolated, with no obvious signs of recent or ongoing major mergers or tidal disturbances. The overall visual impression is that of a quiescent system, likely with low levels of current star formation.
