The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a high degree of central concentration, with a bright, well-defined core. The galaxy's light distribution is quite uniform and its spheroidal shape appears almost perfectly round. There is no evidence of spiral arms, dust lanes, or other features typically associated with disk galaxies. The galaxy displays a yellow/orange hue, indicative of an older stellar population with little ongoing star formation. There are no obvious signs of tidal disturbances or interaction with other galaxies in its immediate vicinity. The galaxy seems to be a fairly isolated and relaxed system.
