This galaxy appears to be a spiral galaxy, possibly an intermediate type between a pure spiral and a lenticular. A disk is visible, though it is not sharply defined. There is a central bulge which is small relative to the size of the disk and appears fairly smooth.

There appears to be a blueish tint, indicating star formation, although it may be at a low rate. The spiral arms, though not well-defined, show some signs of disturbance, possibly due to minor gravitational interactions. These disturbances include irregular arm structure and clumpy regions within the arms. Some regions of dust and gas appear near the spiral arms, though these are very faint. The galaxy does not appear to be undergoing a major merging event, but may have experienced a minor merger event.