The galaxy presents a prominent spiral structure, appearing face-on relative to our line of sight. Two well-defined spiral arms emanate from a central bulge, with moderately tight winding. The arms exhibit clumpy regions suggestive of active star formation. The central bulge appears substantial and of moderate size. The overall morphology suggests a possible barred spiral, but the bar is not distinctly visible. There is no obvious sign of tidal disturbances or a major ongoing merger.
