The galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated core that is yellow-white in color. There is evidence of a surrounding disk or envelope that is bluer in color. This bluer region appears fainter and more diffuse than the core. The galaxy exhibits an elongated shape, appearing more 'in-between' rounded and cigar-shaped, with a distinct major axis. There is no obvious evidence of spiral arm structure, and it appears relatively undisturbed, without significant signs of ongoing merging activity or major tidal disturbances. The overall color suggests a stellar population that includes older stars in the core, with possible ongoing star formation in the bluer outer regions.
