The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a bright, intense core that gradually diminishes outwards. The color gradient suggests an older stellar population, primarily appearing in yellowish hues, indicative of evolved stars. There is no clear evidence of spiral arm structures or significant dust lanes. Minor disturbances cannot be completely ruled out but are not readily apparent. Overall, the galaxy appears as a relatively undisturbed, evolved system.
