The galaxy presents as a spiral galaxy, observed at an inclined angle relative to our line of sight. Prominent spiral arms are visible, showing a distinct winding pattern. The arms appear relatively tightly wound near the central bulge and loosen as they extend outward. The galaxy has a clear bulge, with a yellow hue indicating an older stellar population. The disk shows a blue tint, suggesting ongoing star formation within the spiral arms. The arms exhibit some degree of patchiness, possibly indicative of star-forming regions or dust lanes. The overall morphology suggests a well-defined spiral structure. The galaxy appears undisturbed, showing no apparent signs of major mergers or significant tidal interactions. There may be a weak bar structure in the central region.
