The galaxy presents a generally smooth morphology, with a dominant, centrally concentrated light distribution. It appears largely elliptical in shape, with a high degree of roundness. There is a slight hint of disk structure within the galaxy. The color profile suggests a population dominated by older stars, with an overall redder hue. There is evidence of a few redder knots of intense star formation, which are dwarfed by the primary population of older stars. No major disturbances or signs of ongoing merger activity are readily apparent. Faint tidal features are absent.
