The galaxy presents as an edge-on spiral, with a prominent, extended disk bisecting the image. A central bulge is visible, appearing relatively smooth and with a slightly rounded shape. The disk exhibits a color gradient, shifting from bluer hues at the outer edges to redder tones towards the bulge, potentially indicative of differing stellar populations and dust distribution. There is no apparent evidence of significant tidal disturbances or ongoing major mergers. The galaxy exhibits a redder color overall, particularly towards its central regions. There is a lack of clumpy star forming regions, which is also consistent with a low star formation rate.
