The galaxy presents as an elliptical form, with a high degree of central concentration. Its overall color appears somewhat redder, indicative of an older stellar population. The surface brightness profile decreases smoothly outward from the core, showing no distinct features like spiral arms or a prominent disk. There is a slight elongation to the galaxy's shape, suggesting it is either a flattened elliptical or possibly a lenticular galaxy seen at an angle. No significant dust lanes or active star-forming regions are discernible in this image. Based on its morphology, a significant rate of on-going star formation is not expected. The galaxy's apparent smoothness suggests a relatively relaxed dynamic state.