The galaxy presents a clear spiral structure, with arms emanating from a central bulge. The bulge appears moderately sized and exhibits a yellowish hue, suggesting a population of older stars. Two prominent spiral arms are visible, wound moderately tightly around the bulge. These arms are not uniformly colored; they display variations in brightness and color, indicating regions of active star formation interspersed with older stellar populations. The overall color of the spiral arms is bluer than the bulge, consistent with the presence of younger, hotter stars. The galaxy disk is inclined relative to our line of sight. There is no apparent major disturbance or signs of a major ongoing merger event, though the spiral arms exhibit some asymmetries, possibly due to minor gravitational interactions or internal processes. A faint bar is visible in the center of the bulge, bisecting it.
