The galaxy presents as a relatively smooth, elliptical morphology, with a highly concentrated central bulge and a diffuse halo. There is no clear spiral arm structure apparent. The color gradient suggests a moderate level of star formation occurring within the galaxy, with a slightly bluer tint surrounding the central bulge. There are no obvious signs of a major ongoing merger or tidal disruption events, though subtle disturbances cannot be ruled out. Based on its ellipticity, it is close to being in between round and cigar shaped.
