The galaxy appears as a single, centrally concentrated object. The morphology is smooth, lacking prominent spiral arms or other distinct features. It's roughly circular in shape, with a slight elongation. The color is generally yellowish-orange, suggesting an older stellar population. There is no apparent dust lane or strong evidence of ongoing star formation discernible from the image. The galaxy does not appear to be undergoing a major merging event, although some minor asymmetry hints at possible past interactions or internal disturbances.
