The galaxy presents as a flattened, disk-like structure with an elliptical profile. Its central region exhibits a high surface brightness, appearing almost uniformly luminous with a yellowish hue. Surrounding the core is a fainter, bluish disk that appears somewhat clumpy, hinting at possible spiral arm structures that are not well-defined. There is some indication of dust lanes or irregular features within the disk. The overall color distribution suggests active star formation is occurring, particularly in the outer regions, based on the observed bluer color. No obvious signs of a major ongoing merger are apparent.
