The galaxy presents a largely smooth, elliptical morphology. A concentrated, luminous core is visible, transitioning into a more diffuse halo. The color profile suggests a relatively evolved stellar population. There is a hint of bluer light in the outer regions indicating ongoing star formation. No spiral arm structure or prominent dust lanes are discernible. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. It is mostly round, and likely an early-type galaxy.
