The galaxy presents a predominantly blue hue, indicative of ongoing star formation. A central, somewhat brighter region suggests the presence of a galactic bulge, although it doesn't dominate the overall structure. Multiple spiral arms are visible, displaying a winding pattern. The arms exhibit a mix of medium and loosely wound configurations, creating a complex structure. The galaxy shows signs of tidal interactions or recent minor mergers, evident from the slightly distorted morphology and irregular distribution of star-forming regions within the arms. The disk is not viewed edge-on. Overall, the galaxy appears to be an actively star-forming spiral system undergoing some form of gravitational interaction, leading to disturbances in its morphology.
