The galaxy presents as a relatively smooth, elliptical structure, elongated along its major axis. The central region exhibits a concentrated luminosity, appearing yellowish-white, suggesting a population of older stars. The outer regions display a gradual decline in brightness, with a faint greenish-blue hue, which could indicate areas of more recent, though not particularly vigorous, star formation. The overall morphology indicates a system that is likely not undergoing any major mergers or disturbances, presenting as a fairly evolved galaxy.
