The galaxy appears to be a relatively undisturbed, elongated spiral galaxy, seen edge-on. A central bulge is visible, exhibiting a yellowish hue, suggesting a population of older stars. The disk shows a bluer color profile toward the outer edges, potentially indicative of ongoing star formation within spiral arms, though these arms are not clearly resolved in this image. The galaxy is not perfectly symmetrical, and seems to possess an "In Between" roundness, indicating a transition between a perfectly round and a more elongated shape. Overall, the galaxy presents a smooth appearance with the spiral components blending together because of the high viewing angle. There seems to be a high degree of uniformity in its composition, possibly suggesting a lack of recent major merger events. The galaxy is distant, evidenced by the observed redshift.
