The galaxy appears to be a relatively smooth, centrally concentrated system. Its morphology is predominantly elliptical, exhibiting a high degree of circularity. There is no discernible spiral arm structure or prominent disk component. A slight asymmetry is noted. The galaxy's light profile suggests a somewhat uniform distribution of stellar populations. A trace level of internal disturbance is present, potentially resulting from a minor interaction with another galaxy. There are is little if any dust absorption visible. 
