The galaxy appears as a relatively smooth, centrally concentrated object, exhibiting a largely elliptical morphology. There is a lack of distinct spiral arm structures. The overall color profile suggests a bias towards redder wavelengths. This, in combination with the smoothness, suggests an older stellar population with relatively low current star formation. There is also a slight elongation to the structure. A mild irregularity is observed on one side, suggesting the possibility of a minor gravitational interaction or internal disturbance. No signs of any major merger are apparent. 
