The galaxy presents an elliptical morphology, appearing largely featureless and smooth in its overall structure. The light distribution is centrally concentrated, with a gradual decrease in surface brightness extending outwards from the core. There is a subtle color gradient, transitioning from a yellowish-orange core to slightly bluer hues in the outer regions. The smooth profile suggests a lack of significant ongoing star formation, indicating a more evolved stellar population dominating the galaxy's luminosity. No evidence of spiral arms, dust lanes, or tidal features is discernible.
