The galaxy appears to be a relatively smooth, elliptical system with a centrally concentrated luminosity profile. There may be a faint disk or faint features present, but the system is dominated by the smooth, spheroidal component. The color distribution suggests a population of older stars, likely with minimal recent star formation. The galaxy's shape is fairly round. No signs of tidal tails or strong gravitational disturbances are visible, although there is a possibility of a minor disturbance given the slight asymmetry in its outer isophotes. There is an apparent neighboring galaxy in close proximity.
