The galaxy presents as a generally smooth, elliptical structure with a concentrated central bulge. The color distribution exhibits a radial gradient, transitioning from a yellow-white core to a reddish halo. This suggests an older stellar population dominates, with a possible decline in star formation activity. The overall shape is somewhat irregular, showing a slight deviation from perfect sphericity, appearing to be more in-between, not quite round but not significantly elongated. There is no clear evidence of strong tidal interactions or major mergers. Subtle disturbances or minor interactions may be occurring based on the slight asymmetry. Based on the colors, this galaxy is likely massive.