This galaxy presents as a somewhat elliptical structure with a smooth, featureless appearance. The central region exhibits a yellowish hue, suggesting an older stellar population and a lower rate of current star formation. A greenish-blue halo surrounds the core, potentially indicating a population of younger, hotter stars or ionized gas, but the smoothness of this region suggests it is more likely an older population as well. There's no evidence of spiral arms, bars, or other distinct features typically associated with disk galaxies. The overall morphology suggests an early-type galaxy, likely an elliptical or lenticular galaxy, with minimal signs of recent interaction or significant star formation. A slight red shift indicates that this galaxy is relatively distant from our own. There may be some minor disturbances, but overall it looks like a singular mass.