The observed galaxy presents as a highly elongated, edge-on spiral galaxy. A prominent central bulge is visible, which appears somewhat diffuse and elongated along the major axis. The disk component is very thin, with notable dust lanes obscuring portions of the galaxy. The color is predominantly reddish-orange, suggestive of an older stellar population and potentially significant dust extinction within the disk. There is little evidence of distinct spiral arm structure or active star formation regions within this image. The galaxy exhibits a smooth, symmetrical profile, and no signs of tidal disturbances or ongoing mergers are apparent in the image.
