The galaxy presents as a slightly elongated spheroid with a smooth, concentrated central bulge. There is no readily apparent disk structure; the light distribution appears mostly uniform, fading gradually from the core. The primary color of the galaxy is a pale blue-white, which could indicate the presence of intermediate age or old star populations. A small area of redder light is observed, this could indicate a localized region of older stars or dust extinction. Overall, the galaxy appears to be relatively undisturbed, lacking the irregular features associated with recent major mergers or significant tidal interactions.
