The galaxy presents as a disk galaxy, viewed at a considerable inclination.  A central bulge is visible, appearing moderately sized. This bulge appears yellowish, suggesting an older stellar population. The disk component shows a spiral structure, though the arms are tightly wound and somewhat indistinct, giving it a somewhat flocculent appearance. There are hints of multiple spiral arms emanating from the central bulge, seemingly with two or three prominent arms.  The spiral arms exhibit a bluer color, indicative of ongoing star formation.  Dust lanes appear to be present along the inner edges of the spiral arms, partially obscuring light from behind.  The overall shape of the galaxy is elongated, with a relatively high ratio of major to minor axis. There is no obvious evidence of a strong bar structure. There do not appear to be any major signs of a recent merger or tidal disturbance.
