The galaxy presents as a flattened, disk-like structure when observing the available image. It shows a primarily smooth appearance with a subtle suggestion of spiral arm features or similar internal structures. The central bulge seems moderately defined but not overly prominent.

Color gradients exist within the galaxy. The core exhibits a bluer hue, potentially indicating a higher concentration of younger, hotter stars, while the outer regions trend slightly redder, which could point to an older stellar population or increased dust obscuration. The galaxy appears to be undergoing a minor gravitational interaction with another galaxy. A slight bridge or distortion is visible on the edges of the galaxy. It may be undergoing a merger, but only minorly.
