The galaxy appears as a moderately luminous, concentrated object, generally elliptical or spheroidal in shape, with a smooth light distribution. A slight elongation is discernable along its major axis. The color profile appears to be a relatively uniform yellow-orange, indicative of an older stellar population. There may be a possible very slight disturbance in structure indicative of a minor tidal interaction or past merger event, but the galaxy is mostly undisturbed. There is no clearly evident disk or spiral arm structure.
