The galaxy presents a largely smooth morphology, exhibiting minimal discernible features like spiral arms or a prominent disk structure. It has an elliptical or possibly lenticular shape, appearing mostly rounded but also slightly elongated. The central region displays a high concentration of luminosity, suggesting a significant stellar density. The color appears predominantly red-yellow, which could be indicative of an older stellar population and suppressed star formation within the galaxy. There is no obvious evidence of any recent or ongoing mergers or tidal disturbances. Faint, diffuse light extends from the center, fading into the background sky.
