The galaxy presents as a system of three interacting or closely associated components. The primary, central component exhibits a smooth, elliptical morphology. The light from this component peaks in the yellow-orange wavelengths. Based on the roundness of the galaxy, it is classified as generally round. 

A secondary component is located southwest of the primary. This component appears bluer in color.

A third, fainter component is located east of the primary and is redder in hue. 

Given the disturbances suggested by the presence of the three components, a significant fraction of light may be emitted because of star formation. The system is likely undergoing or has recently undergone a minor merger event.
