The galaxy presents as a centrally concentrated object with a somewhat spheroidal morphology. The core exhibits a reddish hue, possibly indicating an older stellar population, or significant dust obscuration. A fainter, greenish-blue emission extends outwards from the center. This could be indicative of ongoing star formation in the outer regions, though the resolution is insufficient to resolve distinct star-forming regions. No prominent spiral arms or bar structures are discernible. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or nearby companion galaxies. The overall appearance is consistent with a relatively massive galaxy.
