The observed galaxy presents a generally smooth and elliptical morphology. The light profile appears highly concentrated toward the center, with a relatively rapid decline in surface brightness as radial distance increases. The galaxy exhibits a dominant yellowish-red color, possibly indicating an older stellar population and a lower rate of on-going star formation. There are no obvious spiral arms or significant dust lanes visible, nor any indication of recent or ongoing merger activity. The overall structure suggests an evolved system, possibly a large elliptical galaxy.
