The galaxy presents as an elliptical or lenticular type. The light is concentrated towards the center. The galaxy exhibits a smooth appearance with a high degree of central concentration, and with a relatively symmetrical, rounded shape and has a noticeable bulge. There is a lack of obvious spiral arm structures or dust lanes. Color gradients suggest a concentration of older stellar populations and a small amount of on-going star formation. The red shift indicates the galaxy is at an intermediate distance. The image suggests the galaxy is a relatively massive system. Evidence indicates that the system is not undergoing any major merging events or disturbances.
