The galaxy presents a generally smooth, elliptical morphology. The central region appears to be dominated by an older stellar population, exhibiting a yellowish-orange hue indicative of evolved stars. There is a subtle gradient in color and intensity moving outward from the core, with the outer regions appearing slightly fainter. No distinct spiral arm structures or dust lanes are discernible. The galaxy's shape is approximately circular with minimal elongation. There are no obvious signs of ongoing or recent major mergers. The galaxy exhibits a relatively high degree of symmetry and homogeneity in its light distribution.
