The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. The galaxy exhibits a radial gradient in color, with a more yellowish-white core and a redder, fainter halo. No distinct spiral arm structures are discernible. There's a very slight asymmetry, with the halo appearing slightly more extended on one side. The smoothness implies an older stellar population, lacking in substantial ongoing star formation. Evident is the galaxy’s evolved state, with minimal signs of recent mergers or major disturbances.
