This galaxy exhibits a distinct spiral structure. The arms are well-defined and extend outwards from a bright central bulge. While the disk is not perfectly edge-on, there is no evidence of a bar structure. The central bulge appears moderate in size, with an elliptical shape and a smooth texture, which is characteristic of older stellar populations. Overall, the galaxy is dominated by a fairly smooth structure, while some arms are apparent. There is no strong evidence for major merging activity. The presence of distinct spiral arms suggests ongoing star formation within the disk. 
