The galaxy presents a prominent spiral structure, exhibiting well-defined arms that emanate from a central bulge. These arms display a mixed morphology, with some appearing tightly wound while others are more loosely structured. The galaxy's color gradient suggests a distribution of stellar populations; the central bulge exhibits a yellowish-orange hue, indicative of older, redder stars, while the spiral arms show bluer regions, likely locations of ongoing star formation. Dust lanes appear to be present within the spiral arms, obscuring some of the starlight. The overall appearance suggests a relatively undisturbed disk galaxy with active star formation regions. There are no signs of a major ongoing merger, but a minor disturbance cannot be ruled out. The galaxy appears to be at a considerable distance, given the observed redshift, and is of substantial size.
