The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. The light distribution appears relatively uniform across the main body of the galaxy, lacking prominent spiral arm structures or distinct features. The core region is characterized by intense luminosity, suggesting a significant concentration of stars. There is little visual evidence of on-going star formation within the galaxy; overall color indices suggest a predominantly older stellar population. The galaxy exhibits a round shape. Evident within the image is a lack of major disturbances that would indicate an ongoing or recent major merger event. The light is slightly more red than blue, and appears very faint.
