The galaxy presents as a spiral type, observed at an intermediate inclination angle relative to our line of sight. Prominent spiral arms extend from a central bulge, with a moderate bulge size relative to the disk. The spiral arms exhibit a primarily medium winding, with flocculent structure. A possible bar-like structure appears to cut through the center of the galaxy. No major signs of disturbance from recent mergers are visible in the disk. The central bulge appears to exhibit higher luminosity than the disk. Star formation appears to be actively occurring within the spiral arms. There appear to be two main spiral arms, but there is also some evidence of a third.
