The galaxy presents as a relatively compact object. It exhibits a generally smooth morphology with no apparent spiral arm structures or significant dust lanes visible. The galaxy appears nearly circular in shape, showing minimal elongation. Color gradients across the galaxy are subtle, with a slightly bluer core region and a gradually redder halo, suggesting potential variations in stellar populations or dust content across its radial profile. There is no obvious tidal debris, suggesting the system hasn't undergone recent major merger activity, though the presence of subtle irregularities in the outer halo cannot be ruled out given the image resolution.
