The galaxy presents as a concentrated, spheroidal system with a smooth light distribution. The central region exhibits a bright, yellowish-orange hue, suggesting an older stellar population dominated by redder stars. There is a subtle color gradient, transitioning to a slightly greenish-yellow halo extending outwards. No distinct spiral arms or prominent dust lanes are discernible. The overall morphology indicates a relatively undisturbed system, likely an elliptical galaxy or a lenticular galaxy viewed face-on. There is no apparent evidence of recent major merger activity or strong tidal disturbances.
