The galaxy presents as a flattened, elliptical morphology, viewed nearly edge-on. A bright, concentrated central bulge dominates the structure, exhibiting a yellowish-white hue indicative of an older stellar population. Surrounding the bulge is a fainter, broader disk. The disk displays a greenish tint, potentially suggesting ongoing star formation or a population of younger, bluer stars. There is a slight asymmetry in the overall shape, with hints of possible tidal features extending subtly from the main body of the galaxy. These could be indicative of past gravitational interactions or minor disturbances. The disk appears relatively smooth, lacking prominent spiral arm structures or distinct dust lanes. There are subtle color gradients present within the disk region, indicating variations in stellar populations or dust content across the galactic plane.
