The object appears to be a spiral galaxy, viewed at an angle somewhat between face-on and oblique. Evident spiral arm structure is present, though not sharply defined. The arms appear flocculent. There is a definite central bulge, which appears substantial and of moderate size relative to the galactic disk. The galaxy exhibits a blueish hue in the disk region, suggesting recent or ongoing star formation. The overall structure suggests a galaxy that has not experienced any major recent mergers, but possibly minor interactions as suggested by the arm structure. There is no clear evidence of a strong bar structure.
