The galaxy presents as a flattened, disk-like structure viewed nearly edge-on. A prominent central bulge is evident, appearing smoothly rounded and concentrated. The disk component exhibits a noticeable dust lane bisecting the galaxy along its major axis, obscuring a portion of the light from the stars behind it. No signs of recent or ongoing major mergers are visibly apparent in the image, nor are strong tidal features such as tails or bridges. Minor disturbances might be subtly present within the disk, though these are not obvious at this resolution. The overall color profile suggests a mix of stellar populations, with bluer regions possibly indicative of recent star formation. Given its edge-on orientation, determining the presence of spiral arms or other detailed disk features is difficult, but there is no apparent structure.
