The galaxy presents as an elliptical form, with a bright, concentrated central bulge. A diffuse halo surrounds this central region, gradually fading into the background sky. There is a slight asymmetry in the halo's extension; perhaps a minor tidal interaction. The color gradient suggests a predominantly older stellar population. Limited color variation is observed within the galaxy, indicating either a lack of significant ongoing star formation, or obscuration by dust. The galaxy displays features of disturbance.
