The galaxy presents as a relatively compact, elliptical-like structure. The core region exhibits a high degree of concentration of light, indicative of an older stellar population, appearing yellowish-orange in color. Moving outward from the center, the light intensity diminishes gradually, displaying a smooth, diffuse halo without prominent spiral arms or distinct features. There are hints of blue tinges, indicating areas of younger star formation. However, these appear subdued, suggesting a low to moderate current star formation rate, but with a high stellar mass. No significant signs of tidal disturbances or ongoing major merger events are observed, although there appears to be some form of disturbance in the outer regions. The overall morphology suggests a system in a relatively quiescent evolutionary stage.
