The galaxy presents a smooth, elliptical morphology with a concentrated, bright central bulge. The galaxy is relatively round, displaying minimal disk-like features. There is a clear radial color gradient, transitioning from a yellowish core to a redder halo. The absence of distinct spiral arms or significant dust lanes suggests a relatively evolved system with a low rate of on-going star formation. There appears to be no major merging event currently in progress. The overall structure suggests a galaxy that is primarily supported by random stellar motions rather than rotation, which would be consistent with its apparent elliptical shape.
