This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity extending outward from the core. The galaxy is generally round in shape with no distinct features such as spiral arms or a bar apparent. There is a suggestion of color variation, with a slightly redder hue near the center, possibly indicating an older stellar population, transitioning to a slightly bluer periphery. This blue-shifted light could be attributed to a population of younger stars or a recent episode of star formation. There is no evidence of any major disturbances or ongoing mergers.
