The galaxy presents a prominent disk structure with spiral arms. These arms display a tightly wound morphology, indicating differential rotation. The central bulge is moderately sized and appears yellowish-white in color, suggesting a significant population of older stars. The spiral arms themselves exhibit a bluer hue, indicative of ongoing star formation. The arm count is difficult to discern due to the image resolution and arm winding but appears to be 1-4 arms. The galaxy does not appear to be edge-on and shows no sign of a strong central bar. The morphology suggests the galaxy is not undergoing any major merging events, although there might be some minor disturbances.
