The galaxy presents as a largely smooth, elliptical structure. It exhibits a high degree of central concentration, with luminosity decreasing radially from a bright, nearly circular core. The color profile is generally redder in the central regions, transitioning to slightly bluer hues in the outer halo, suggesting a potential population shift from older to younger stars with increasing radial distance. There is little indication of significant spiral arm structure or active star formation regions discernible in this image. The overall morphology indicates a system that has likely undergone significant dynamical relaxation and quenching of star formation. There appear to be no major mergers or tidal disruptions presently affecting the galaxy's morphology, though minor disturbances cannot be completely ruled out. The light distribution suggests a generally spheroidal shape, with minimal elongation or asymmetry.
