The galaxy appears as a single, relatively smooth object. Its morphology leans towards elliptical, with a high degree of central concentration. The galaxy presents a nearly circular shape.

The core exhibits a yellow hue, with hints of green on the periphery. The galaxy's overall color suggests an older stellar population, although the traces of green could indicate some ongoing, albeit minimal, star formation. The lack of distinct spiral arms or a well-defined disk is consistent with a system dominated by older stars. There are no obvious signs of a major ongoing merger, although the possibility of minor tidal disturbances cannot be entirely ruled out given the low resolution. The galaxy appears relatively undisturbed and isolated.
