The galaxy appears to be a spiral galaxy, though the structure is somewhat disturbed. There is a faint but noticeable disk structure present, however the arms are not well-defined. It's face-on to our line of sight. There is no dominant central bulge. There is some evidence of ongoing star formation, indicated by the slightly bluer color in some regions of the disk. Irregularities in the shape suggests some sort of interaction and/or tidal disturbance. The galaxy has a moderate stellar mass. Overall, it seems to be a late-type spiral galaxy experiencing some level of activity and/or merging.
