The galaxy presents as a relatively smooth, centrally concentrated object. The core region exhibits a yellowish hue, suggesting an older stellar population. There may be an intermediate age population also present given the greenish light. There are a few reddish regions, perhaps signaling star formation or dust extinction. The morphology is generally elliptical to slightly oval, with no strong evidence of spiral arms. There is a small red smear along one of the sides. It appears to be an isolated galaxy with no clear signs of major disturbances or ongoing mergers.
