The galaxy presents a generally smooth and rounded morphology. The central region displays a concentrated brightness that appears yellowish-white in color. This suggests a likely older stellar population dominating the core. Surrounding the bright center is a more diffuse, bluish halo. The blue hue indicates the presence of younger, hotter stars potentially formed through recent or ongoing star formation. The lack of a distinct spiral arm structure or bar suggests that this galaxy may be classified as an elliptical or lenticular galaxy. There is a slight asymmetry in the outer halo, however the image does not present signs of major mergers. The relative smoothness points towards an evolved system with less active star formation in the galactic center compared to the outer edges.
