This galaxy appears to be a relatively smooth, elliptical galaxy. It is characterized by a concentrated, bright central bulge, transitioning to a fainter, more diffuse halo. The color gradient suggests the presence of older stellar populations, with a yellow/orange hue concentrated in the central region and slightly bluer colors in the outer regions. This galaxy exhibits a slight elongation, appearing more "in between" round and cigar-shaped, as opposed to perfectly spherical. There is no obvious evidence of significant spiral arm structure or major mergers, although there may be subtle signs of minor disturbances in the outer regions. The overall structure indicates a relatively evolved system.