The galaxy presents an elliptical morphology, appearing as a moderately elongated spheroid. The core exhibits a pronounced luminosity, indicating a concentration of stars and likely a supermassive black hole at its center. The galaxy displays a smooth profile, with no prominent spiral arm structures or significant dust lanes visible. There are slight disturbances, such as very faint wisps surrounding the main body, indicating minor gravitational interactions. Color gradients suggest older stellar populations, evidenced by the reddish hues dominating the central region. Overall, the galaxy appears to be a massive, evolved system with a relatively low star formation rate.
