The galaxy presents an edge-on morphology, appearing as a flattened, elongated structure. The central region exhibits a bright, concentrated bulge, with a notably rounded form. Diffuse light extends outwards from the bulge, indicative of a disk component. The disk appears relatively smooth, lacking prominent spiral arm structures. Dust lanes or significant obscuration are not clearly visible within the disk. The galaxy displays a colour gradient, trending from a yellowish-white core to slightly bluer hues in the outer regions of the disk. The overall colour suggests a relatively evolved stellar population, although the bluer outer regions may indicate ongoing or recent star formation. No signs of major mergers or significant tidal disturbances are apparent. There might be a very faint disturbance to the left side of the galaxy but it is not certain from this image. The galaxy is well-defined and symmetrical, with a smooth appearance, implying a dynamically stable system.
