The galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated bulge. The light distribution is relatively even with a slightly elliptical shape. There is minimal evidence of spiral arms or dust lanes within the galaxy. The color indices suggest a population of older stars, as indicated by the redder hue. There are no obvious signs of recent or ongoing major mergers, though there is a subtle asymmetry in the outer regions which may indicate a minor interaction. The galaxy exhibits a fairly high degree of central concentration.
