The galaxy presents a disk-like morphology with spiral arm structures. A central bulge is visible. The spiral arms appear somewhat flocculent, exhibiting a patchy distribution of star formation regions. There is a possible bar structure. The galaxy shows no significant signs of major mergers or extreme tidal disturbances, although there is some minor indication of such activity. The galaxy's disk is not perfectly edge-on, but shows an inclination, with the spiral arms being visible. The color suggests ongoing star formation.
