The galaxy appears to be a spiral galaxy, presenting a face-on orientation relative to our line of sight. Prominent spiral arms are clearly visible, extending outward from a central bulge. These arms exhibit a somewhat loosely wound morphology. A bar-like structure appears to be present traversing the galactic center. The bulge displays a moderate size relative to the overall galactic disk. Color gradients are observable within the spiral arms, suggestive of ongoing star formation. The galaxy does not exhibit any major signs of significant merging activity, though a slight asymmetry within the arms might suggest some minor past interaction. Two main arms appear to be prominent.
