The galaxy presents as a spiral type, displaying prominent, albeit tightly wound, spiral arms. The arms exhibit a complex structure with varying degrees of definition, suggesting differential star formation rates across the galactic disk. The central bulge appears substantial, exhibiting a moderate degree of luminosity concentration, indicating a likely supermassive black hole at its center. The overall color profile suggests a mix of stellar populations, with bluer tones potentially indicating younger, actively star-forming regions within the spiral arms, and yellower tones potentially indicating a higher concentration of older stars, particularly within the central bulge. There appears to be no obvious signs of any major on going merger, but some minor irregularities in the disk structure could indicate past or present interactions. The galaxy's disk appears to be close to face-on, allowing for a more unobstructed view of its spiral structure.
