The galaxy presents a generally smooth and elliptical morphology. The light distribution suggests a high degree of central concentration with a gradual decline in surface brightness outwards from the core. A yellow-orange hue dominates the central region, potentially indicating an older stellar population. The outer regions appear slightly bluer, possibly due to younger stars. There appears to be a subtle hint of a faint disk. There is no strong indication of spiral arm structure or significant dust lanes. Overall, the galaxy appears relatively undisturbed, without major signs of mergers or tidal interactions.
