The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. Its color is predominantly yellow-red, indicating an older stellar population with fewer young, massive stars. The isophotes appear generally round, with no obvious spiral arm structure or bar features visible. There is no discernible evidence of ongoing major mergers or significant tidal disturbances in its immediate vicinity. The galaxy is relatively compact and has a high degree of central concentration. It is likely to be a massive galaxy with a high mass and a low star formation rate.
