The galaxy appears to be an elliptical or lenticular type, displaying a largely smooth and featureless morphology. A bright, concentrated central bulge is evident, which gradually fades into a more diffuse halo. There is minimal evidence of spiral arm structure or prominent dust lanes. The overall color profile suggests an older stellar population with a lack of significant ongoing star formation. The shape approximates a flattened spheroid. There is possible minor tidal disturbance in the halo of the galaxy. 
