The galaxy presents as a spiral, exhibiting a predominantly face-on orientation. Its central bulge appears relatively small to moderate in size, emitting a bright, concentrated light. Spiral arms are clearly visible, displaying a tightly wound morphology. Faint and fuzzy, difficult to discern exact number of spiral arms. No bar structure apparent at the center. Evidence of disk-like structure. Disk appears to be undergoing star formation. Overall the disk features light, with an otherwise smooth profile, and a fairly symmetrical shape. There are a few dust lane features within the disk. No obvious signs of major mergers, but some indications of minor disturbances in the galaxy's morphology. The overall color profile suggests a mix of stellar populations, with blue hues in the arms potentially indicating regions of active star formation and redder tones in the central regions suggesting older stellar populations.
