The galaxy presents as a largely featureless, smooth object with a concentrated central bulge. It appears nearly circular, displaying only a slight deviation from perfect roundness. There is little evidence of spiral arms or a distinct disk structure. Color gradients suggest a redder core transitioning to a bluer outer region, potentially indicative of an older stellar population concentrated centrally and younger stars towards the periphery. There are no obvious signs of ongoing major merger activity or significant tidal disturbances, although subtle asymmetry cannot be entirely ruled out. The galaxy's overall appearance is consistent with an elliptical or an early-type spiral galaxy viewed at a considerable distance.