The galaxy presents a spiral morphology, although the spiral arms are not sharply defined. There is evidence of ongoing star formation, as suggested by the relatively blue color. The galaxy appears to be relatively large. It exhibits a bar structure. The central bulge is prominent, but does not dominate the galaxy's overall appearance. There is no apparent major merger or significant disturbance to the galaxy's structure. The galaxy appears relatively isolated in its environment, with no other major galaxies in close proximity.
