The galaxy presents an elongated, roughly elliptical morphology. It shows a prominent central bulge that exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter, bluer regions are present in the outer disk, indicating the presence of younger, hotter stars and potential star-forming regions. The disk appears to be viewed at an oblique angle. There is a hint of a dust lane or obscuration along the galactic plane, which could indicate a warped or disturbed disk. Some minor tidal features are visible in the form of faint diffuse extensions, indicating a possible past interaction with another galaxy.
