The object presents as a spiral galaxy with a redshift indicating intermediate distance. The galaxy exhibits a prominent disk structure. Spiral arms are clearly visible and appear to be relatively tightly wound around the central bulge. The color of the spiral arms suggests the presence of younger, bluer stars, indicative of ongoing star formation. The central bulge displays a yellowish hue, potentially indicating an older stellar population. There is evidence of a bar structure. The overall morphology suggests a well-defined spiral structure, with no immediately apparent signs of major mergers or significant tidal disturbances. The galaxy's color indices suggest moderate levels of star formation activity, with a relatively high specific star formation rate. The appearance of the disk indicates that it is being viewed at more of a face-on angle, and not edge-on.
