The galaxy presents as a spiral, observed at a slight angle relative to face-on. There is a central bulge. The bulge appears moderate in size and exhibits a yellowish color, suggestive of an older stellar population. The spiral arms are prominent and well-defined. These arms display a bluish hue, indicating ongoing star formation. The arms appear tightly wound around the central bulge. The overall morphology suggests a system that is currently undergoing active star formation within the spiral arms while maintaining a relatively well-defined structure. There are no obvious signs of major interactions or mergers.
