The object presents as a relatively bright, face-on spiral galaxy. A prominent central bulge appears yellow, suggesting an older stellar population. Spiral arms are clearly visible, exhibiting a bluer hue indicating ongoing star formation. The disk of the galaxy is not perfectly circular but exhibits a slightly elliptical shape. The galaxy displays a well-defined structure, and no major signs of ongoing interaction or merger events are immediately apparent. There is some evidence for a weak bar structure in the central region. The galaxy is a spiral. The galaxy shows a gradual decrease in brightness from the core to the outer regions.
