The galaxy presents a predominantly smooth morphology, appearing largely featureless in the available image. There's a subtle elongation to its shape, possibly deviating slightly from being perfectly circular. The galaxy exhibits a color gradient, appearing bluer in the outer regions and redder towards the center, possibly indicating the presence of older stellar populations concentrated towards the galactic core. There is no noticeable spiral structure or bar. There are no signs of a major ongoing merger, although it could have experienced minor interactions. The galaxy is compact with a concentrated light profile. 
