The galaxy presents as a moderately sized, elliptical or lenticular structure with a central bulge that appears quite bright and concentrated. The light distribution suggests a relatively smooth profile, although some subtle irregularities and faint extensions can be discerned in the outer regions. The core exhibits a strong concentration of light, indicating either a dense stellar population or a possible active galactic nucleus. The overall color is yellowish-white, implying an older stellar population with fewer young, massive stars. Faint plumes or tidal features are possibly present, hinting at a past interaction or merger event.
