The observed galaxy presents as a relatively faint, edge-on disk galaxy. The disk appears quite thin, showing a relatively symmetrical structure. A central bulge is not clearly prominent, appearing fairly small relative to the disk. Patches of differing luminosity across the disk suggest variations in star formation or dust obscuration. Some subtle asymmetries in the disk may point to minor interactions. The color appears bluer along the edges of the disk, possibly indicating the presence of younger stars in the spiral arms. There is a distinct lack of prominent spiral arm structure. There may be ongoing or recent minor merger activity due to the morphological disturbances, but no clear signs of tidal tails or disrupted morphology are seen.
