The galaxy presents as a centrally concentrated, smooth object with a dominant spheroidal component. The light is mostly homogenous with an apparent gradual increase in luminosity towards the core. There is a slight elongation of the central region along an axis. The galaxy appears to be yellowish-white in color, indicative of an older stellar population. A very faint disk component may be present, but the spheroid dominates. There are no obvious signs of ongoing major mergers or tidal disturbances. The overall impression is that of a relatively relaxed, early-type galaxy.
