The galaxy presents a well-defined spiral structure. Two prominent spiral arms emanate from the central region. The arms appear somewhat flocculent, and the winding is intermediate, being neither tightly wound nor loosely structured. The central bulge is modest in size relative to the disk. There is no pronounced bar feature apparent in the central region. The color gradient suggests that the central region is more red than the outskirts. There are no obvious signs of a major merger, but there appears to be a minor disturbance or potential companion galaxy that is gravitationally interacting with the main galaxy, deforming one of its arms. This minor disturbance or small companion galaxy may be the cause of the deformation of one of the galaxy's spiral arms, while the other arm is undisturbed. The galaxy is not edge-on; it is observed at an angle that allows a clear view of the spiral arms.
