The galaxy presents as a generally smooth, elliptical morphology. It has a bright, concentrated central bulge which appears slightly yellow. Moving outward from the center, the galaxy diffuses into a fainter halo that is less uniform in color. The halo exhibits subtle mottling, suggesting some structural inhomogeneity. Overall, the light distribution is quite symmetric and centrally concentrated. There is no clear evidence of spiral arms or a distinct disk structure. It seems to be a galaxy that is relatively quiescent, showing little evidence of major recent mergers or active star formation.
