The galaxy presents as an elliptical or lenticular type with a smooth, centrally concentrated light distribution. There's a discernible core region exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. The overall shape appears somewhat elongated, but not highly so, transitioning from a more concentrated nucleus. No prominent spiral arms or distinct dust lanes are visible in this image, consistent with a classification leaning towards earlier-type galaxies. The galaxy's extended halo shows a subtle blueish tint, which might suggest ongoing, albeit mild, star formation activity, or could be light from younger stars scattered by dust. The galaxy does not appear to be strongly interacting with any other visible galaxies and shows only some minor disturbance, though it is located in a field with a high density of other galaxies.
