The galaxy appears to be a relatively large, elliptical galaxy. It presents a smooth, centrally concentrated luminosity profile with no readily apparent spiral arms or disk structure. The galaxy's shape is neither perfectly spherical nor significantly elongated, but is rather an oval shape. The galaxy's color indices suggest a population of older stars, though some younger stars may be forming. The galaxy does not appear to be undergoing any major merging activity or significant tidal disturbances, though some small distortions may be present.
