The galaxy presents as a centrally concentrated system with a bright, nearly circular core region that gradually fades into the outer regions. There appears to be little spiral structure, rather the galaxy shows a generally elliptical morphology. The colour profile suggests a population of older stars, indicated by the yellowish-red hue throughout much of the galaxy. The outer regions are smoother and more diffuse. The overall appearance is consistent with an early-type galaxy such as an elliptical or lenticular galaxy. There is very little evidence of active star formation. The object exhibits a high degree of central concentration.
