The galaxy appears as a slightly elongated, disk-shaped structure. There's a hint of spiral arm structure visible, though somewhat faint and patchy, suggesting a flocculent or poorly defined spiral pattern. The central region is relatively smooth and possibly contains a bulge. The overall color of the galaxy leans towards blue, suggesting the presence of younger, hotter stars and ongoing star formation. However, there is also evidence of redder regions. This could indicate the presence of older stellar populations or dust lanes within the disk. There also seem to be some minor disturbances, with possibly some distortions to the galaxy's structure. This is likely due to gravitational interactions with another galaxy.
