The observed galaxy exhibits a well-defined spiral structure. It presents a central bulge with a moderate size, surrounded by a relatively flattened disk. Two prominent spiral arms are clearly visible, exhibiting a medium winding pattern around the galactic center. There appears to be a weak bar structure extending through the center of the galaxy. The overall morphology suggests a lack of significant interaction or recent merger events, with only minor indications of disturbance in the galactic disk. Star formation appears to be moderate, as suggested by the subtle blue color, indicating active regions of star birth within the spiral arms. The galaxy is viewed at an angle that allows the spiral structure to be seen, but not perfectly face-on, nor edge-on.