The galaxy presents as a largely amorphous, diffuse object. The overall color appears to be a yellow-orange hue, suggestive of an older stellar population dominating its light output. There is little to no discernible spiral structure, and no distinct features such as dust lanes or star-forming regions are apparent. The light is centrally concentrated and fades into the background sky in all directions with no sharp boundary. There is no obvious tidal debris or signs of recent merger activity. This galaxy likely has a substantial mass, but a low star formation rate. Its appearance indicates that it is likely an elliptical galaxy.
