The galaxy presents as a relatively smooth, centrally concentrated elliptical or lenticular system. It exhibits a bright, well-defined nucleus surrounded by a diffuse, elliptical halo of light. There is little evidence of spiral arm structure, dust lanes, or significant star-forming regions visible within the resolution of the image. The color appears predominantly yellow/orange, which suggests an older stellar population with a lower rate of current star formation. The galaxy appears undisturbed, with no obvious signs of recent mergers or tidal interactions.
