The galaxy presents as a somewhat elliptical structure, with a generally smooth appearance. The central region exhibits a higher surface brightness, appearing as a concentrated bulge. This region transitions into a fainter, more diffuse halo that extends outwards. There is a slight suggestion of a disk component, although it is not sharply defined. The galaxy's color profile indicates a population of older stars. There is no obvious signs of ongoing major merger activity or strong tidal disturbances. Minor disturbances can not be ruled out. The overall structure appears relatively undisturbed, suggesting a system that has undergone significant dynamical relaxation.
