The galaxy presents a somewhat smooth, elongated morphology. It appears as a disk galaxy viewed at an oblique angle, close to edge-on. The central bulge exhibits a higher concentration of light compared to the outer regions of the disk. Some internal structure is subtly visible within the disk, though the overall appearance suggests a relatively mature system. The galaxy is inclined with a position angle that places it at approximately 122 degrees. There's a hint of a slightly bluer color in the disk, potentially indicating ongoing star formation. The isophotes show moderate flattening. There are no obvious signs of major disturbances or interactions, although the smoothness of the galaxy does not preclude minor disturbances. HI properties suggest cold gas content.
