The galaxy presents a clear spiral structure. Two prominent spiral arms emanate from a central bulge, winding moderately outwards. A bar-like feature appears present, bisecting the bulge region. The bulge exhibits a yellowish hue, indicating a population of older stars. The spiral arms are bluer, suggesting ongoing star formation. The size of the bulge is moderate relative to the overall galactic disk. There is no obvious indication of a major merger event, but some minor disturbances may be present in the outer disk. The spiral arms are tightly wrapped.
