The galaxy appears as a centrally concentrated object, with a generally elliptical morphology. A bright, reddish-yellow core transitions into a more diffuse, greenish halo or extended disk. The isophotes appear mostly smooth, indicating a lack of prominent spiral arms or distinct features. There is a slight elongation of the galaxy along one axis, suggesting it is not perfectly circular. Visual inspection does not indicate any major disturbances or ongoing merger events, although there may be subtle asymmetries within the halo. The smooth appearance suggests a relatively relaxed, dynamically evolved system.
