The galaxy presents an elongated, disk-like morphology. It is oriented approximately horizontally in the image. The central region appears brighter and more diffuse, suggesting a higher concentration of stars and interstellar material, likely a bulge. The color gradient indicates bluer hues at the outer edges of the disk and more yellow/red hues near the center. This could be due to the presence of younger, hotter stars in the spiral arms, and older, cooler stars in the bulge.

There are irregularities in the light distribution suggesting some internal structure, though defined spiral arms are not obviously visible at this resolution. The overall appearance could indicate an edge-on or highly inclined spiral galaxy. The galaxy shows no obvious signs of a major merger, but subtle irregularities may suggest minor gravitational disturbances. The galaxy appears relatively isolated and undisturbed.
