The galaxy presents a generally smooth, elliptical morphology with a notable central concentration of light. There is a slight elongation observed, with the major axis oriented roughly northwest to southeast. The galaxy exhibits a radial gradient in luminosity, with brightness decreasing smoothly outwards from the core. The color appears relatively uniform, indicating a lack of strong color gradients across the galaxy. No distinct features such as spiral arms, dust lanes, or prominent star-forming regions are discernible within the available data. The overall appearance is consistent with a relatively old stellar population and minimal ongoing star formation.
