The galaxy presents as a flattened, elongated structure, suggesting a disk galaxy viewed nearly edge-on. A prominent central bulge is observed, appearing smooth and concentrated. The bulge exhibits a noticeable yellowish-white hue, possibly indicating an older stellar population. Fainter blue light emanates from the disk, potentially indicating regions of younger, hotter stars. The overall smooth appearance of the galaxy suggests it is relatively undisturbed, without signs of major ongoing mergers or tidal distortions. There is a slight asymmetry in the light distribution along the major axis, although no distinct features indicative of star formation regions are apparent.
