The galaxy appears to be a spiral galaxy, likely of late-type, viewed at an oblique angle, but not quite edge-on. A disk-like structure is visible, with a suggestion of spiral arms, although distinct arm features are not readily apparent from this image resolution. The central bulge appears relatively small and indistinct. The galaxy exhibits a blue hue overall, suggesting ongoing star formation. There are regions of brighter blue light scattered throughout the disk, likely indicating areas of enhanced star formation activity. There is a slight indication of possible minor disturbance in its structure, but no major merger event appears to be occurring. The galaxy is not a perfectly smooth, featureless object, and it exhibits some degree of internal structure within its disk component.
