The galaxy presents an elongated, lenticular morphology, viewed edge-on. A prominent central bulge exhibits a reddish-orange hue, indicative of an older stellar population and/or significant dust obscuration. The disk component, extending beyond the bulge, displays a bluer color, possibly due to more recent star formation and a younger stellar population. The disk appears relatively thin and has a clear symmetry. Overall, the galaxy exhibits a smooth profile, lacking prominent spiral arms or irregular features.
