The galaxy appears to be a spiral type, though the arms are not sharply defined. A central bulge is clearly visible, exhibiting a yellowish hue, suggesting an older stellar population. The spiral arms have a bluish tinge, indicative of ongoing star formation. The arms appear somewhat tightly wound, and not overly flocculent. No obvious signs of major disturbances or ongoing mergers are observed. The galaxy is relatively well-defined, with a smooth overall appearance. There seems to be a moderate disk size with a smaller bulge.
