The galaxy presents an elliptical morphology, appearing largely smooth in texture. It exhibits a concentration of yellow light toward its core, suggesting an older stellar population dominates the central region. Surrounding the core, a more diffuse, greenish-blue halo extends outwards. This color may indicate regions of recent, albeit relatively low, star formation occurring within the galaxy’s outer reaches. There are no readily apparent spiral arms or significant dust lanes. The galaxy's overall shape is close to circular, with only a slight elongation discernible. There is no obvious evidence of any recent major merger events; it appears to be a relatively undisturbed system. Some small disturbances can't be ruled out.
