The galaxy presents as a largely smooth, elliptical structure, with a generally rounded morphology. A bright, concentrated central bulge is evident. There are no apparent spiral arms or a distinct disk component discernible in the image. The galaxy exhibits a subtle color gradient, appearing more reddish towards the core and slightly bluer towards the outer regions. No signs of major mergers or significant tidal disturbances are readily observed, though some minor asymmetries may be present within the galactic halo. The overall appearance suggests a relatively evolved galaxy, consistent with a population of older stars.
