The galaxy presents as a relatively smooth, elliptical-like structure. A diffuse central bulge is visible, exhibiting a brighter concentration of light compared to the outer regions. There's a subtle color gradient, transitioning from a bluer core to slightly redder hues in the outskirts, which could indicate differential stellar populations or dust distribution. The object does not display any prominent spiral arms or distinct features indicative of active star formation. There might be a very faint, ill-defined disk component, but it's difficult to ascertain with certainty from the image alone. Overall, the morphology appears to be that of a galaxy evolving towards a more quiescent state.
