The galaxy presents as a largely smooth, elliptical-like object, approximately circular in projection. The luminosity profile appears centrally concentrated with a gradual decline outward from the core, suggesting a lack of distinct spiral arms or disk features. There is a subtle color gradient, appearing slightly more yellow-red toward the center. The overall color suggests an older stellar population, possibly indicating low ongoing star formation. There is no clear evidence of recent merger activity or major disturbances in its morphology. The structure is largely homogenous and well-defined.
