This galaxy presents as a spiral type, with a prominent central bulge and a visible disk structure. The spiral arms are apparent but tightly wound, exhibiting a relatively smooth texture and a distinct lack of clumpy star-forming regions. The arms appear somewhat flocculent, with no single dominant arm structure. The galaxy is observed face-on. A bar is potentially present, though its structure is not pronounced. There is no indication of any major merger event; however, there is some evidence of minor interaction based on the somewhat disturbed outer regions of the disk. The central bulge appears to be of moderate size in relation to the overall galactic structure. The bluer color of the disk suggests ongoing star formation, albeit likely at a moderate rate.
