The galaxy presents as a spiral type, exhibiting a disk-like morphology. Prominent spiral arms are discernible, wound at a moderate pitch angle. The central bulge is visible, appearing to be of moderate size compared to the disk. There is a suggestion of a bar-like structure within the central region, though not distinctly defined. The overall color suggests evolved stellar populations, showing a yellow-red hue throughout the galaxy. Evidence of active star formation, indicated by blue regions, is observed along the spiral arms. There is an indication of an ongoing interaction or merging event with a smaller galaxy or companion object. The disk is viewed at a low inclination. 
