The galaxy appears to be a spiral galaxy with a prominent, moderately sized bulge. Two well-defined spiral arms emanate from the central bulge. The spiral arms exhibit a medium winding, appearing relatively tightly wound. The galaxy's disk is viewed nearly face-on. Evidence of a bar structure is present, but it is not particularly pronounced. The galaxy displays no obvious signs of major interaction or significant disturbance, appearing relatively undisturbed. Star formation appears moderate and centered in the spiral arms.
