The galaxy appears to be a spiral galaxy, oriented somewhat face-on relative to our line of sight, exhibiting a pronounced disk structure. Spiral arms are visible, although somewhat diffuse and flocculent. The arms appear to be moderately wound. The central bulge is of moderate size. The overall color suggests ongoing star formation, with hints of bluer regions within the spiral arms. There is no obvious bar structure present. The galaxy shows no clear evidence of strong tidal interactions or major merging activity, although minor disturbances cannot be ruled out. The galaxy exhibits a redshift, placing it at a significant cosmological distance.
