The galaxy presents as a well-defined elliptical or lenticular structure. It exhibits a smooth, centrally concentrated light profile, with minimal evidence of spiral arms or prominent dust lanes. The color appears relatively uniform across the galaxy, suggesting a stellar population that is primarily composed of older stars, with reduced on-going star formation. The galaxy's shape is somewhat elongated, falling somewhere between completely round and a more elongated "cigar" shape. There appear to be signs of potential past interaction or minor disturbances, although no major merger is immediately obvious in the image.
