The galaxy presents as a spiral galaxy, oriented roughly face-on with a moderate inclination. The spiral arms are well-defined. The winding of the arms appears to be somewhat mixed, with some portions exhibiting a tighter wind while others show a looser configuration. The central bulge region is prominent, exhibiting a strong concentration of older, yellower stars. The overall color suggests ongoing star formation, particularly within the spiral arms where patches of bluer light are observed. There is a clear disk structure. There is a lack of evidence for any major or minor mergers; this galaxy appears to be isolated with no noticeable tidal features or distortions in its morphology.
