The galaxy presents as a relatively face-on spiral, although the spiral arms are not sharply defined. A central bulge is evident, appearing with a yellowish-white hue, indicative of an older stellar population. Surrounding the bulge, the galaxy exhibits a bluish tint, suggesting the presence of younger, hotter stars within the spiral arms. These arms are not distinct, but rather appear as a more diffuse distribution of star formation. The overall morphology suggests a disk galaxy with some degree of internal structure, but without significant morphological disturbances that would indicate a recent major merger event. The galaxy is neither completely smooth nor strongly featured. There's a hint of a disk-like structure, but it's viewed at an angle that's not quite edge-on. Evidence of any significant merging events is not readily apparent, though minor disturbances may be present.
