The galaxy presents as a relatively smooth, centralized structure with a dominant, elliptical morphology. A discernible color gradient is visible, with a brighter, more yellowish core transitioning to a slightly redder outer halo. The galaxy appears largely undisturbed, without any prominent tidal features, major asymmetries, or indications of an ongoing major merger event. The roundness of the galaxy suggests it has a morphology closer to an elliptical galaxy. The limited evidence of blue light may suggest a relatively low ongoing star formation rate, or a galaxy population with a bias towards older stars. The visual impression is that of a mature galaxy, likely with a significant stellar mass.
