The galaxy presents as a fairly smooth, elliptical-like object with a concentrated central bulge. The light is dominated by a yellowish-orange hue, suggesting an older stellar population. There is a slight hint of bluer light peripherally, potentially indicating some ongoing, albeit limited, star formation in the outer regions. The galaxy appears relatively undisturbed, showing no clear signs of ongoing major mergers or tidal interactions. Its overall roundness suggests a system that has reached a degree of dynamical equilibrium.
