The galaxy presents as a relatively compact, luminous structure with a moderate degree of smoothness. The overall form appears to be neither perfectly elliptical nor clearly spiral, showing properties somewhere in between. It is generally round. The color profile indicates a redder, and therefore older stellar population, with very little discernible blue light associated with ongoing star formation. There are indications of minor disturbances within the galaxy, suggesting that there may be some sort of merger, or interaction taking place.
