The object appears to be a spiral galaxy exhibiting a relatively face-on orientation with a redshift indicating a moderate distance. The spiral arms are well-defined and extend outwards from a somewhat ill-defined central bulge. There's a flocculent structure evident in the spiral arms, with variations in luminosity along their length. The arms appear to be relatively tightly wound around the central bulge, with hints of a multi-armed structure. The colour profile suggests ongoing star formation, particularly in the spiral arms, indicated by the blueish hue. There may be a weak bar structure present across the central region. Overall, the morphology of this galaxy suggests it is likely a late-type spiral galaxy, classified somewhere between Sb and Sc. The relative lack of significant dust lanes is also notable. There is no obvious signs of recent or ongoing major merger activity, although there appears to be minor asymmetries in the spiral arm structure.