This galaxy exhibits a clear spiral morphology, displaying prominent, tightly wound arms. A central bulge region is visible, appearing somewhat moderate in size. The disk is viewed at an angle, less than perfectly edge on. Dust lanes appear to be present throughout the disk, partially obscuring starlight. The overall color suggests a mix of stellar populations, with a bluer tint in the spiral arms and a yellower hue concentrated towards the bulge, potentially indicating older stars. There appears to be no signs of any major merger events happening. There seems to be star formation occurring within the spiral arms of this galaxy. 
