The galaxy presents as an elliptical morphology, showing a smooth, diffuse light distribution. The core exhibits a yellowish-orange hue, suggesting an older stellar population, potentially dominated by evolved stars. Extending outward from the central region, there's a gradual transition to a bluer color, hinting at the presence of younger, hotter stars in the outer regions. The disk is noticeably inclined relative to our line of sight, evidenced by its elliptical projection on the sky. There are no prominent spiral arm structures or dust lanes visible, consistent with its classification as an elliptical galaxy. The smooth light profile indicates a relatively quiescent galaxy with minimal ongoing star formation outside the central regions.
