The galaxy presents a generally smooth and elliptical appearance, though it may be exhibiting some disk-like qualities. It appears to be a relatively evolved system with a bright central bulge and a diffuse halo. The axial ratio suggests the galaxy is more in-between round and cigar shaped, with a slight elongation. No major disturbances or ongoing mergers are readily apparent, indicating a period of relative quiescence. Star formation appears to be relatively low, or has been quenched, giving the galaxy redder magnitudes.
