The galaxy presents as a relatively compact object. It exhibits a bright, concentrated central region suggesting the presence of a galactic bulge. The overall light distribution appears somewhat smooth, although there is indication of some asymmetry in the outer regions. There may be very faint and subtle distortions or extensions along the galaxy's periphery, hinting at possible minor gravitational interactions. It is not clear whether these are genuine structural features or artifacts. Color gradients are observed, with the central region appearing bluer than the outer halo.
