The galaxy presents as a flattened, disk-like structure seen nearly edge-on. A prominent central bulge appears with a yellowish-orange hue, suggestive of an older stellar population. The disk exhibits a bluer color, potentially indicating ongoing star formation, however, the disk region is quite faint with some patchy light distribution. The overall morphology appears relatively undisturbed with only a few signs of tidal features or significant asymmetry. Based on its color and morphology, this galaxy can be classified as a spiral galaxy of medium size and mass. The low level of disk light could indicate an older stellar population.