The galaxy presents as a spiral type, observed at a relatively face-on angle. Two main spiral arms are visible, exhibiting a moderate winding. These arms display a blue hue, indicative of active star formation regions containing young, hot stars. A central bulge is present, appearing a yellowish color, suggesting an older stellar population within. The bulge is of moderate size in comparison to the overall disk. There is no clear evidence of a strong bar structure bisecting the galaxy. No major mergers or significant tidal disturbances are apparent in this image, but a minor disturbance cannot be ruled out. The galaxy possesses a defined disk.