The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology with a high degree of roundness. There is little evidence of spiral arms or a pronounced disk structure. Color gradients are apparent, with a more blueish hue towards the central region that diffuses outwards into a yellowish and reddish halo. There is a very slight suggestion of a disturbance in the galaxy shape, but it is difficult to ascertain whether the object is merging with another galaxy or is simply experiencing some sort of internal perturbation.