The galaxy exhibits a prominent disk structure with observable spiral arms. The arms appear tightly wound. A bulge is present, but it is not the dominant feature. The galaxy appears to have two relatively tightly wound spiral arms. There is evidence of a bar structure spanning the central region of the disk. The colour of the galaxy suggests it contains a mixture of stellar populations, with the bulge and inner disk exhibiting a yellowish hue and spiral arms exhibiting a bluish tinge. The overall structure does not appear to be significantly disturbed, suggesting it is not currently undergoing a major merging event.
