This galaxy exhibits a relatively smooth and rounded morphology. It presents a centrally concentrated brightness profile, appearing more luminous towards its core. There is a subtle color gradient observed, transitioning from a bluer central region to slightly redder outer areas. No distinct spiral arms or prominent disk features are discernible. The overall appearance suggests a system that is not undergoing significant merging or major disturbances. The shape is largely elliptical with a large smooth fraction. The luminosity indicates substantial size and mass. The inferred star formation rate suggests a moderate level of ongoing stellar birth within the galaxy.
