The galaxy presents as a somewhat diffuse, centrally concentrated object with a generally smooth appearance. Its overall shape appears largely elliptical or spheroidal, displaying a high degree of roundness, showing minimal deviation from a circular form. 

There are no prominent spiral arms or a distinct disk structure visible. There appears to be a slight asymmetry in the outer regions, potentially indicative of a minor gravitational interaction or disturbance, but it is difficult to say definitely from this image.

The galaxy does not exhibit any strong signs of ongoing major merger activity. It seems to be mostly a singular object. The core has a smooth, consistent color profile, showing a central bulge structure.
