The galaxy appears as a relatively compact, elliptical or lenticular system with a smooth, centrally concentrated light distribution. There is no obvious spiral arm structure or dust lane obscuration visible. The color gradient suggests a generally older stellar population, with a slightly redder hue dominating the galaxy's light. The galaxy's shape appears close to circular. There's no apparent tidal debris or other indications of recent major merger events. The faintness of the outer regions suggests it is a galaxy of moderate luminosity and mass.
