The galaxy presents a largely smooth and elliptical morphology, exhibiting a concentrated central bulge. The light distribution appears relatively even and symmetrical. There is no readily apparent structure such as spiral arms or a prominent disk. Color gradients suggest the central regions may be composed of older stellar populations with a redder hue, transitioning to a bluer tint in the outer regions, indicative of younger stars. The overall color index suggests ongoing, albeit potentially declining, star formation activity. There are no signs of strong tidal interactions or major disturbances in the galaxy's shape, implying it has likely undergone no recent major mergers. It exhibits a rounded shape, showing minimal elongation. The luminosity of the galaxy implies a substantial stellar mass.