This galaxy exhibits a clear spiral structure. Two distinct spiral arms emanate from a central bulge. These arms appear grand design, and loosely wound. The bulge is moderately compact and displays a yellowish hue, indicative of an older stellar population. Blue hues dominate the spiral arms, suggesting ongoing star formation. There appears to be no strong bar structure visible across the galaxy's center. The galaxy is not obviously undergoing a major merger, though there may be minor disturbances in the outer disk. The disk itself is viewed nearly face-on. Overall, the galaxy presents as a well-formed spiral with a mixture of older and younger stellar populations.
