The galaxy presents as a spiral type, with a noticeable disk structure inclined somewhat from a face-on orientation. Spiral arms are apparent, extending from the central region, which seems to possess a moderately sized bulge. The arms display a rather loose winding, and the presence of two distinct arms is observed. Areas of possible active star formation are hinted at by the patchy distribution of brighter regions within the arms. There is evidence of minor disturbance, perhaps due to a weak interaction or merger event. The disk appears to be relatively flat, and not observed as edge on. A weak bar structure may be present. The overall color suggests ongoing star formation activity.