The galaxy presents as a relatively compact and moderately luminous object. Its morphology appears to be largely smooth, displaying a centrally concentrated light profile. While there is some suggestion of asymmetry in its outer regions, the dominant impression is that of an elliptical or lenticular system. There is a possibility of minor disturbances within the galaxy, but there is no strong evidence of a major merger event or tidal interactions. The overall color suggests a mature stellar population.
