The galaxy presents as a centrally concentrated object with a smooth, featureless morphology. It appears approximately elliptical in shape, with a slight elongation. The light distribution is centrally bright, diminishing gradually outwards. The galaxy exhibits a color gradient, with a bluer hue towards the core and a subtly redder tone in the outer regions. No distinct spiral arms or bar structures are discernible within the limits of the image resolution. There is no apparent evidence of ongoing major mergers or significant tidal disturbances.