The galaxy presents as a largely smooth, centrally concentrated object. The overall morphology is generally round. There is a slight elongation in the morphology, though the round fraction is dominant. There is no clear evidence of spiral arms or a prominent disk structure. Color gradients are visible, trending from a bright, potentially older population in the core to a bluer halo region suggesting younger star formation. No significant signs of tidal disturbances or ongoing major merging events are apparent, though the presence of subtle irregularities cannot be entirely excluded.
