The galaxy appears to be an edge-on spiral, with a prominent, elongated disk structure bisecting the image. A central bulge is evident, exhibiting a yellowish hue suggestive of an older stellar population. The disk shows a bluer tint, indicative of more recent star formation activity. The disk appears relatively smooth, with no clearly resolved spiral arm structures visible at this resolution. The galaxy's light is more concentrated towards the center, with intensity gradually diminishing toward the edges of the disk. There is a degree of dust lane obscuration. Overall, the galaxy exhibits a flattened morphology with a relatively high degree of axial symmetry.
