The galaxy exhibits a morphology indicative of a spiral galaxy with a central bulge. It is observed at a redshift that suggests a relatively close distance. There is evidence of ongoing or recent star formation activity, as suggested by the galaxy's color, tending towards the blue end of the spectrum. The disk of the spiral is inclined at an angle that allows for a clear view of the spiral arms. These arms appear somewhat flocculent. Although somewhat faint, there is evidence of a bar-like structure spanning the central region of the galaxy. Overall, the galaxy displays a complex structure with evidence of both ordered rotation and some degree of dynamical disturbance possibly due to a minor merger or tidal interaction. The apparent size is relatively small, indicating that the galaxy is either intrinsically compact or viewed at a substantial distance. The galaxy displays characteristics of a relatively high mass, with significant star formation.
