The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The overall color gradient suggests a higher concentration of older stellar populations, indicated by the yellowish hue, particularly toward the core. There is a subtle fading and a possible hint of a disk-like structure present at its edges, though it's not a highly prominent feature. There is no clear evidence of spiral arms or strong dust lanes, indicating a passively evolving system. There are no major disturbances or signs of ongoing mergers. It exhibits a regular, rounded shape.
