The galaxy presents as a concentrated, centrally brightened system. It exhibits a dominant, smooth spheroid component with a noticeable yellow hue, suggesting a relatively older stellar population in the core. There is evidence of a faint, diffuse disk surrounding the central bulge, showing a hint of bluer regions, indicative of younger stars or ongoing star formation. The overall shape appears to be somewhere in between round and elliptical. There is no clear indication of major mergers or strong tidal features, but the outer regions are somewhat asymmetrical, possibly suggesting minor gravitational interactions or internal disturbances.
