The galaxy presents as a relatively smooth object, possibly elliptical in morphology. The light distribution appears concentrated toward the center, suggesting a prominent bulge. The overall color is yellowish-white, indicative of an older stellar population and a lack of significant ongoing star formation. There is a slight elongation in the morphology, but the galaxy generally appears rounded. No distinct spiral arms or features are visible. There is no strong evidence of any recent or ongoing merger activity or major disturbances. The overall appearance suggests a galaxy that has largely completed its star formation and is evolving passively.
