The galaxy presents as a slightly elongated, disk-like structure. Its color gradient suggests a higher concentration of older stars towards the center, indicated by the reddish-yellow hue. Moving outward, the disk appears to fade, showing a less defined boundary. The overall morphology seems more akin to a somewhat smoothed distribution of light, lacking sharply defined spiral arms or a prominent central bulge. The axial ratio suggests a significant inclination relative to our line of sight. There is a hint of some sort of minor disturbance but nothing significant.
