The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. It appears elliptical, exhibiting a high degree of radial symmetry. There is a pronounced color gradient, shifting from a bright, yellowish core to a fainter, redder halo. No distinct spiral arms, dust lanes, or other features characteristic of disk galaxies are discernible. The light distribution suggests an older stellar population dominates. There is no evidence of recent or ongoing mergers or major tidal disturbances.
