The galaxy presents as a moderately redshifted, elongated system. Its morphology appears to be largely smooth, with some suggestion of a disk-like structure. The central region exhibits a yellowish hue, possibly indicative of an older stellar population or dust obscuration. Fainter, bluish extensions are visible along the major axis, potentially representing regions of younger star formation. There is a suggestion of minor disturbances in the overall morphology, but it does not appear to be undergoing a major merger event. The galaxy's axial ratio is quite high, suggesting it is viewed at a significant inclination angle. The color gradients suggest a radial change in stellar population or dust distribution.
