The galaxy presents as a spiral type, observed at an oblique angle, not quite edge-on. There is a clear disk component with discernible spiral arms, although the image resolution limits detailed tracing. The arms appear relatively tightly wound. A central bulge is present, exhibiting a moderate size relative to the overall disk. The bulge shows a yellowish hue suggesting an older stellar population. The disk component displays a bluer tint indicative of ongoing star formation. Evidence of a bar structure is present, based on the subtle elongation of the bulge and a somewhat rectangular morphology in the inner regions of the disk. No obvious signs of major mergers or significant tidal disturbances are apparent in the galaxy's morphology.
