The galaxy presents as an edge-on spiral, exhibiting a flattened, disk-like structure. A prominent central bulge is apparent, showing a smooth, concentrated light profile, suggesting a significant population of older stars. The disk appears relatively uniform in color, with a slight blueish hue towards the outer regions, suggestive of ongoing star formation. There's no noticeable presence of strong dust lanes or significant disturbances in the disk, indicating it is relatively stable and unperturbed. The overall morphology is consistent with a galaxy that has undergone significant disk formation, and is largely dominated by evolved stellar populations.
