This galaxy presents as a spiral, exhibiting a well-defined disk structure. The arms are tightly wound around a central bulge, that appears rather small in comparison to the overall size of the galaxy. They extend outwards, tracing a grand design spiral pattern. The color gradient suggests active star formation within the arms. The spiral arms contain intricate dust lanes and regions of enhanced brightness, potentially indicating areas of concentrated star formation. The central bulge exhibits a smoother, yellowish hue, possibly indicative of an older stellar population. There is no obvious sign of a major ongoing merger, though some subtle asymmetries in the outer disk could suggest minor gravitational interactions or disturbances in the past. Based on its orientation, the galaxy is observed nearly face-on.
