The galaxy presents as a largely elliptical structure with a smooth, diffuse light distribution. The central region exhibits a high concentration of light, appearing almost spherical. A color gradient is discernible, transitioning from a warmer, yellowish hue in the core to a cooler, slightly bluer tone in the outer regions. There may be faint evidence of a disk but is hard to discern, indicating a spheroidal shape. No clear signs of spiral arms or strong dust lanes are apparent. There is some visual evidence of minor disturbance in the galaxy shape.
