The galaxy appears to be a spiral galaxy, observed at a moderate redshift. The disk shows evidence of spiral arm structure. The arms appear somewhat flocculent rather than grand design. The central bulge is prominent and moderate in size, exhibiting a yellowish hue, suggesting a population of older stars. The disk appears bluer, indicative of younger stars and ongoing star formation. The galaxy has a bar structure running through its center. There is no strong evidence of any major merging or tidal disturbances, although there may be some minor asymmetry. The galaxy is not viewed edge-on.
