The galaxy presents as a centrally concentrated system with a smooth light profile. It is neither distinctly spiral nor elliptical in appearance, but it appears slightly oblong. The central region exhibits a bright, concentrated luminosity, likely associated with a galactic bulge. No distinct features, such as spiral arms, dust lanes, or star-forming regions, are readily apparent. The color suggests a relatively evolved stellar population with low ongoing star formation activity. There may be slight irregularities in the outer halo, but it appears largely undisturbed. It shows no obvious signs of major mergers.
