The galaxy presents as a spiral, exhibiting well-defined spiral arms emanating from a central bulge. The bulge appears relatively moderate in size and has an orange color, suggesting an older stellar population with diminished star formation. The spiral arms show a clumpy structure, indicative of ongoing star formation regions, with pockets of blue. The galaxy appears as if it could have a bar structure, although it is not extremely prominent. The overall morphology suggests that the galaxy is not undergoing a major merger, but there may be minor disturbances in the disk. The galaxy seems to have an active star formation rate. The redshift indicates that we are observing this galaxy as it was roughly 2.6 billion years ago.
