The galaxy presents a largely smooth and centralized morphology. Its shape is generally elliptical, appearing moderately rounded in its overall form with a slight elongation. The light distribution is concentrated towards the center, exhibiting a bright central bulge or core. The color profile suggests an older stellar population in the nucleus, indicated by its yellow-orange hue, while the outer regions seem to have a slightly bluer tone implying the presence of some younger stars. Overall, the galaxy appears relatively undisturbed, without prominent signs of ongoing mergers or major tidal interactions. Some small features are potentially observable, though the resolution is low. 
