The galaxy presents as a luminous, centrally concentrated object. The overall morphology appears largely smooth, with little evidence of spiral arms or distinct features that would suggest a disk. There is an extended halo of diffuse light surrounding the central core. The shape appears generally rounded, showing only slight elongation. There is no obvious signs of strong tidal disturbances or a major merger event in progress; however, a hint of asymmetry suggests a possible past interaction or minor disturbance. Color gradients across the galaxy indicates variation in stellar populations, with the central regions exhibiting a yellow or orange hue, possibly due to older, redder stars, and the outskirts appearing slightly bluer. The galaxy's red shift indicates a considerable distance, influencing both its observed size and apparent luminosity. Based on its observed color and morphology, this galaxy could be classified as an elliptical or lenticular galaxy at moderate red shift.
