The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated central bulge, which appears bright yellowish-orange. The outer regions fade into a greenish halo. There is no apparent spiral arm structure or distinct features that would indicate significant recent merger activity, although there may be a minor disturbance to the galactic structure. The overall shape is somewhat rounded, appearing neither perfectly spherical nor highly elongated. The galaxy's color profile suggests an older stellar population with limited ongoing star formation.
