The galaxy presents as a single, concentrated luminous region. It is generally elliptical in shape, with a high degree of central concentration. The galaxy displays a smooth light distribution, with no apparent spiral arm structure or significant dust lanes. The color gradient indicates a possible redder core. This suggests an older stellar population toward the center. There are no obvious signs of tidal disturbances or ongoing major mergers visible in this image, the galaxy appears relatively undisturbed.
