The galaxy presents as a relatively smooth, elliptical-like structure, with a dominant central bulge. It is characterized by a concentrated luminosity profile, lacking prominent spiral arms or distinct features typically associated with disk galaxies. The color appears to be reddish, indicating an older stellar population with a lower rate of ongoing star formation. There might be subtle indications of minor disturbances or asymmetries in the outer regions of the galaxy, but its overall morphology appears settled.
