The galaxy presents a morphology consistent with a late-type spiral. Tight spiral arms are observed and wrap around a large, centrally located bulge. The arms exhibit a high degree of winding, appearing almost flocculent in nature, and are populated by a myriad of HII regions, inferred from their patchy, blue color. The galaxy is not perfectly face-on; it exhibits a slight inclination. There is no significant sign of recent mergers or interactions, although some minor disturbance is possible. The bulge component is substantial. The disk appears relatively smooth between spiral arms, with no prominent dust lanes visible. The colors suggest ongoing star formation. Overall, it looks to be a fairly normal spiral galaxy, with tight winding and a moderate sized bulge.
