The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that gradually fades into a diffuse halo. The galaxy's light profile indicates a high degree of circular symmetry. There are no readily apparent spiral arms or disk-like features visible. The color gradient suggests that the central regions are dominated by older stellar populations, appearing more yellow, while the outer halo shows bluer hues, suggesting the presence of some younger stars. The overall structure indicates a galaxy that is not currently undergoing any major merging events, and is exhibiting a very low star formation rate.
