The galaxy presents as a singular, centrally concentrated object with a generally elliptical morphology. The core exhibits a high degree of luminosity. A faint, diffuse halo surrounds the central region.  There is some evidence of disk-like structure, but the galaxy appears mostly smooth.  Slight irregularities in the outer regions suggest the possibility of minor gravitational interaction or disturbance.  The overall color is red, indicating a stellar population that is relatively old.