The galaxy presents an edge-on disk morphology. A distinct central bulge is observable, exhibiting a slightly elongated, although difficult to discern, structure. The disk component shows a relatively smooth texture with some evidence of dust lanes along the midplane. The galaxy exhibits a noticeable color gradient, trending towards bluer hues in the outer regions of the disk. This suggests ongoing star formation occurring primarily away from the central bulge. There is no obvious evidence of a significant merger event or tidal disturbances.
