The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. Its color is a general yellowish-white, potentially indicating an older stellar population. There's a slight elongation in its morphology but it appears quite rounded. The galaxy shows no strong evidence of spiral arms, bars, or significant dust lanes. There are no immediately obvious signs of a major ongoing merger, although subtle disturbances in its shape may imply a past interaction, or minor disturbance. The galaxy appears relatively isolated in the image. The light profile appears to gradually fade outward from the core, without sharp edges.
