The galaxy presents as a spiral galaxy, viewed edge-on. The central bulge appears small, although moderately bright, exhibiting a yellow-white hue. The disk shows prominent spiral arm structure extending outwards from the bulge. These arms are tightly wound around the bulge. The structure suggests the arms have a high star formation rate, as indicated by their blue color, likely indicating the presence of young, massive stars. The morphology suggests this is a relatively undisturbed galaxy, with no major signs of interaction or merging events. The disk appears smooth and well-defined. The galaxy appears relatively isolated in the image, suggesting it has not recently undergone significant gravitational interactions.
