The galaxy appears to be elliptical, characterized by a smooth, centrally concentrated light distribution. Its color is slightly redder overall, suggesting an older stellar population with reduced star formation activity. The shape deviates somewhat from a perfect sphere, exhibiting a noticeable elongation. There is no discernible spiral structure or dust lanes visible in the image. The galaxy appears relatively undisturbed, lacking any major signs of ongoing mergers or tidal interactions. The light profile decreases smoothly from the center outwards.
