The galaxy presents as a centrally concentrated, relatively smooth structure. The morphology appears elliptical, tending toward round. There is a high concentration of light near the center of the galaxy that fades towards the outer regions. The color profile indicates a redder core region, transitioning to slightly bluer hues in the surrounding halo. There are no obvious spiral arm structures or significant dust lane features present. There are no notable signs of tidal disturbances or ongoing major mergers. The galaxy's star formation rate is relatively low, with the most intense star formation happening in the central region. Overall, the galaxy appears to be a large, evolved system.
