The galaxy presents as a single, fairly symmetrical object. It exhibits a concentrated central region, with the luminosity appearing to decrease gradually with increasing radius. Its hue suggests the presence of an older stellar population, with a smooth, featureless morphology. There is a slight color gradient with the inner core appearing more yellow than the outer regions which tend towards white. There is no evidence of spiral arms or a significant disk component in the galaxy. No signs of tidal disturbances or an ongoing merger are visible, however the morphology of the galaxy hints at a past minor disturbance. The shape of the galaxy is round. 
