This galaxy appears to be a spiral galaxy observed edge-on. A dust lane is prominent, bisecting the galaxy's disk and obscuring the central bulge. The bulge itself appears small, and the spiral arms are not clearly resolved, suggesting a relatively smooth disk component. There is evidence of moderate star formation activity, but there are no obvious signs of major disturbances or ongoing mergers with other galaxies, although some minor disturbances are possible. The galaxy's overall color is consistent with a redshift of around 0.26, indicating a significant distance. It is estimated to have a moderate stellar mass and specific star formation rate.