The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal with a high degree of roundness. There is a concentration of luminosity towards the center, suggesting a prominent galactic bulge. The light distribution indicates minimal, if any, discernible disk structure or spiral arms.

Color gradients within the galaxy are subtle, exhibiting a yellowish hue in the central region, transitioning to a slightly redder shade towards the outer edges. This color suggests an older stellar population dominates this galaxy, and the overall quiescent nature indicates relatively low ongoing star formation. No signs of significant tidal disturbances or ongoing mergers are apparent in this image.
