The galaxy appears as a moderately bright, elliptical object. Its core exhibits a concentrated, yellowish hue, suggesting an older stellar population. The luminosity gradually diminishes from the center outwards, transitioning to a less pronounced greenish halo surrounding the central bulge. This outer region appears relatively smooth, without any apparent distinct spiral arm structures. The overall morphology seems indicative of a relatively undisturbed system, showing no signs of major mergers or tidal disruptions.
