The galaxy presents as a spiral with a prominent, though not dominant, central bulge. Spiral arms are clearly visible and appear tightly wound. The arms exhibit a clumpy structure, suggesting active star formation regions. The color gradient transitions from a yellow/orange hue in the bulge region to bluer colors in the outer spiral arms, consistent with an older stellar population in the center and younger, hotter stars in the arms. There is no obvious presence of a strong central bar structure. The galaxy shows signs of potential disturbance or interaction, possibly minor tidal features or asymmetries in the arm structure that could indicate a past or ongoing merger event. The galaxy appears relatively face-on.
