The galaxy presents as a somewhat elliptical, moderately concentrated object. It appears relatively smooth in texture, without prominent spiral arms or significant dust lanes visible at this resolution. The color gradient suggests a slightly bluer core region, potentially indicative of recent or ongoing star formation, transitioning to redder hues in the outer regions, which could imply an older stellar population. There is no strong evidence of a major ongoing merger, although subtle asymmetries or disturbances in the galaxy's shape cannot be entirely ruled out with this image alone. The overall structure seems relatively quiescent, suggesting a system dominated by settled stellar populations.
