The galaxy appears to be an edge-on spiral galaxy, exhibiting a clear disk structure. A bulge component is faintly visible, though it appears relatively small. The disk shows a distinct color gradient, with bluer hues towards the outer regions and redder colors concentrated towards the central bulge. This may indicate ongoing star formation in the outer disk. The galaxy's disk appears smooth with no clear evidence of prominent spiral arm structures. There may be some obscuring dust lanes along the plane of the galaxy, although not sharply defined. Overall, the galaxy exhibits a relatively regular morphology, suggesting a dynamically evolved state.
