This galaxy presents as a spiral, viewed nearly edge-on. A central bulge is visible, appearing moderately sized and bright. The disk component dominates the galaxy's overall structure. Spiral arms are present, exhibiting a structure that ranges from medium to loosely wound. Evidence suggests two primary spiral arms. A bar feature is apparent, extending across a significant portion of the central region. Overall, the galaxy appears somewhat undisturbed, lacking obvious signs of a major merger event, however, subtle disturbances cannot be ruled out. The galaxy exhibits a measurable redshift, indicating its cosmological distance. Based on the colors, it appears to be actively forming stars.
