The galaxy presents as a spiral type, observed at a moderate redshift. The disk structure dominates the overall morphology, with prominent spiral arms exhibiting a distinct pattern. These arms show a well-defined structure, winding around the central bulge. The winding appears to be primarily of a medium type. A bulge is observed, appearing as a moderate feature.

No significant signs of tidal disturbances or ongoing major merger events are detected in this particular field, though it could be exhibiting minor disturbances. The galaxy is not seen edge-on, but at an angle to the viewing plane allowing for the easy identification of spiral arms.

The central region shows a brighter luminosity, likely indicating a high concentration of older stellar populations, while the spiral arms display a bluer color, suggesting ongoing star formation activity. This is further corroborated by estimates of star formation rate.
