The galaxy presents a smooth, elliptical morphology. The light profile is centrally concentrated with a relatively even distribution. The galaxy appears roughly circular in shape, displaying minimal deviation from radial symmetry. The color index indicates a redder overall color, possibly indicating an older stellar population and/or significant dust obscuration. There are no immediately apparent signs of spiral arms, bars, or tidal features, suggesting the absence of recent major merger events. The object appears to be a fairly massive galaxy with a low star formation rate.
