The galaxy presents as a relatively smooth, elliptical structure with a dominant central bulge. The light distribution indicates a high degree of symmetry and concentration. The core exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer extensions are visible on either side of the central region. There is no discernible spiral arm structure or strong dust lane obscuration. Overall, the galaxy appears to be in a relatively quiescent state, potentially an early type galaxy with suppressed recent star formation. Based on its structure and color, it likely hosts a significant population of evolved stars and a substantial mass.
