The galaxy presents as a face-on spiral with a prominent, moderately sized bulge that exhibits a yellowish hue, suggesting an older stellar population. The spiral arms are clearly defined and feature a predominantly blue color, indicative of ongoing star formation. The arms appear to be relatively tightly wound near the central bulge, transitioning to a medium winding pattern as they extend outwards. The structure of the arms suggests a two-armed spiral galaxy morphology. There are slight color variations across the galactic disk, implying a heterogeneous distribution of stellar populations and dust. The overall appearance indicates a dynamically settled galaxy undergoing active star formation within its spiral arms. There may be a slight perturbation, suggesting a possible minor interaction or merger in its recent past.
