The galaxy presents as a moderately luminous, elongated structure. Its overall morphology appears to be that of a disk galaxy, seen at a significant inclination relative to our line of sight, appearing nearly edge-on. The central bulge is not prominently visible, but there appears to be a slight concentration of light towards the center of the disk. A subtle color gradient is observed, transitioning from a bluer hue on one end of the disk to a slightly redder shade towards the opposite end and central regions. This suggests differential stellar populations or dust obscuration effects across the galactic disk. There are some hints of possible tidal disturbance of galaxy which gives it a very small distorted shape.
