The galaxy presents as a flattened, disk-like structure seen nearly edge-on. A bright, concentrated central bulge dominates the galaxy's luminosity, transitioning into a fainter, more diffuse halo. The color profile exhibits a central concentration of yellow-white light, indicative of an older stellar population within the bulge. Progressing outward from the core, the disk appears to be bluer, hinting at ongoing or recent star formation activity, although this is not immediately apparent via bright emission nebulae. There is a lack of defined spiral arm structure. Dust lanes may obscure portions of the disk, but resolution constraints preclude definitive identification. The galaxy's overall morphology suggests it is likely a lenticular galaxy, although a more precise classification would require higher resolution imaging and spectroscopic analysis.