The galaxy presents as a centrally concentrated, relatively smooth object. Its overall color is notably redder, indicating an older stellar population with a reduced rate of star formation. The light profile suggests an elliptical morphology, appearing generally rounded with no obvious disk-like features or spiral arms. There is no evidence of any major mergers or significant tidal disturbances in its immediate vicinity. Faint light extends around the galaxy, possibly a diffuse halo of stars or intracluster light associated with the galaxy. 
