The galaxy presents as a spiral type, exhibiting a prominent disk structure viewed at a slight angle relative to edge-on. Spiral arms are distinctly visible, displaying a tightly wound morphology across the galactic disk. These arms exhibit a clumpy structure, suggesting ongoing star formation. The central bulge appears relatively small, but distinct, with a yellow-orange coloration, potentially indicating an older stellar population. A weak bar structure may be present within the bulge region. No major signs of tidal disturbance or interaction with other galaxies are readily apparent, although minor distortions are noticeable in the outer arms. The galaxy’s overall color is bluer in the arms and redder in the bulge, consistent with star formation in the disk and an older population in the core.
