The galaxy presents as a moderately bright, disk-shaped structure exhibiting a dominant smooth morphology. The central bulge region is subtly brighter than the surrounding disk, showing a gradual decline in luminosity towards the outer edges. The disk appears to be nearly edge-on from our line of sight, and shows a faint blue tint, possibly indicating ongoing, low-level star formation. There is no indication of a strong spiral structure or major disturbances in the galaxy's overall form, though there is a faint asymmetry in the light distribution.
