The galaxy presents as a flattened, elongated structure, suggesting a disk-like morphology viewed at a high inclination angle. The central region exhibits a concentrated luminosity, potentially indicative of a galactic bulge. The color gradient transitions from a yellowish-white core to more reddish hues in the outer regions, possibly indicating older stellar populations residing further from the core, where the light is redshifted. There is a relatively smooth texture across the visible body with only minor visual disturbances, showing there are no major ongoing mergers with other galaxies.
