The galaxy presents a face-on spiral structure. Two dominant spiral arms emanate from the central bulge region, tracing out a relatively well-defined pattern. The arms display a somewhat medium winding, neither tightly wound nor loosely extended. The central bulge exhibits a moderate size. Dust lanes are subtle within the spiral arms. There is no obvious evidence of a strong galactic bar structure bisecting the bulge. The morphology indicates the galaxy is likely not undergoing a major merger, though the slight asymmetry suggests a possible minor interaction or disturbance.
