The galaxy appears to be a spiral type, exhibiting prominent spiral arms. These arms are somewhat tightly wound around the central bulge. The bulge itself seems to be of moderate size relative to the overall galactic disk. The disk shows some degree of structure and is not entirely smooth. It is possible that some minor disturbances are present within the galaxy, potentially indicating a past or ongoing interaction or merger event. A possible second galaxy is seen to the left, and may be interacting with this one. There is no obvious bar structure visible in the image. The color profile suggests active star formation within the spiral arms.
