The galaxy presents as a relatively smooth, centrally concentrated object, displaying a generally elliptical morphology, tending towards a more rounded appearance. There is a slight elongation, not significantly deviating from circular symmetry. Its color profile reveals a core region that is somewhat redder, grading outward to bluer hues in the surrounding halo. No distinct spiral arm structures or other obvious disk-like features are discernible. Evidences of potential disturbances or interactions, such as tidal tails or distorted shapes, are generally absent, though there might be hints of minor disturbances.
