The galaxy exhibits a flattened, elliptical morphology, suggesting a spiral or lenticular classification. A prominent central bulge is observed, characterized by a high concentration of light and a yellowish hue. The disk component appears to be viewed at an oblique angle, evidenced by the elongated shape. Faint spiral arm structures are suspected, but the resolution of the image makes it hard to confirm. There is no apparent signs of tidal disturbances or ongoing merger events. Overall, this appears to be a relatively undisturbed galaxy.
