The galaxy presents a generally smooth morphology, appearing largely spheroidal in shape. There is a concentration of light toward the center, suggesting a dense core. The galaxy exhibits a yellow-red hue, which could indicate an older stellar population. No distinct spiral arm structures are discernible; rather, the light distribution appears relatively uniform throughout the galaxy's body. The light is primarily concentrated at the center of the galaxy. There is a slight elongation, or asymmetry, but it is nearly circular.
