The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light distribution is generally symmetrical. The core of the galaxy appears bright and has a yellow hue. The outer regions are less distinct and show a gradual decrease in luminosity away from the center. There is minimal evidence of spiral arm structures or significant dust lanes within the galaxy. The overall color profile suggests a population of older stars, with relatively low ongoing star formation. The galaxy appears fairly isolated, showing no clear signs of major interactions or mergers with other galaxies.
