This galaxy appears to be a spiral galaxy viewed at a slight angle, but not fully edge-on. There is a prominent central bulge that exhibits a yellowish hue, potentially indicating an older stellar population. Fainter spiral arms extend from the bulge into the disk. Although the arms appear ill-defined. There appears to be a moderate amount of structure within the disk with some areas of increased brightness that could represent regions of active star formation, although this is not clearly evidenced from color alone. The galaxy's overall color suggests a mix of stellar populations, with a more pronounced concentration of older stars in the central bulge and a younger population in the disk. The galaxy does not show any signs of any major disturbances and appears relatively isolated and unperturbed.