The galaxy presents as a relatively compact, elliptical or lenticular system. Its light distribution appears smooth and centrally concentrated, showing a minimal presence of distinct features such as spiral arms or a prominent disk. The galaxy's color is predominantly yellow-red, suggesting an older stellar population with a limited amount of ongoing star formation. The lack of bluer regions indicates a paucity of young, massive stars. Based on its integrated light, this galaxy appears to be relatively massive. There are no obvious signs of recent or ongoing mergers or major tidal disturbances.
