The galaxy presents as an edge-on spiral, exhibiting a prominent central bulge that appears smooth and concentrated. The disk is clearly visible, though narrow, due to the edge-on orientation. The bulge appears yellowish-white, indicating a population of older stars. The disk displays a bluer hue, suggesting the presence of younger, hotter stars and some ongoing star formation. There are no immediately obvious signs of active galactic nuclei activity or major mergers, although there is the possibility of a minor disturbance. The overall morphology suggests a galaxy that is not currently undergoing intense starburst activity.
