The observed galaxy presents a spiral morphology, exhibiting prominent spiral arms. Two dominant arms are clearly visible. The arms appear loosely wound. A central bulge is present, although it does not seem to dominate the overall structure. There may be a bar structure within the bulge. There do not appear to be any major indications of interactions with any nearby galaxies. The disk of the galaxy is viewed at a slight angle. Star formation seems to be present within the galaxy.