The galaxy exhibits a notably elliptical morphology, appearing somewhat elongated along a particular axis. It is characterized by a smooth, diffuse light distribution, lacking prominent spiral arms or distinct features typically associated with disk galaxies. The central region of the galaxy displays a concentrated brightness, suggestive of a substantial galactic nucleus. The galaxy's color is primarily a warm yellow-orange hue, indicating an older stellar population with a relative scarcity of young, hot, blue stars. There is little evidence of significant dust lanes or active star formation regions within the galaxy. The overall appearance indicates a galaxy that has largely exhausted its supply of gas and dust, resulting in a diminished rate of star formation.
