The galaxy presents as an elongated, disk-like structure seen nearly edge-on. A prominent central bulge exhibits a concentrated yellowish-white color, suggesting an older stellar population. Diffuse extensions are visible above and below the bulge. These areas appear less concentrated and have a bluer hue compared to the central region, which may be due to the presence of dust or gas and associated star formation activity. There are no obvious signs of major mergers or tidal disturbances in the immediate vicinity of the galaxy. The image is not sharp enough to resolve individual stars or star clusters.
