The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light distribution is centrally concentrated and appears to fade gradually outwards. There is an overall yellowish-orange hue, which suggests a population of older stars. The shape is somewhat elongated, though not extremely so. There's no clear evidence of spiral arms or significant dust lanes. There are no major disturbances or signs of an ongoing merger. The galaxy is likely an evolved system with low star formation activity.
