The galaxy appears to be a relatively smooth, round object with a concentrated central bulge. There is a noticeable color gradient, transitioning from a yellowish-white core to a bluer and fainter outer region. The overall morphology suggests a relatively evolved system, potentially an elliptical or lenticular galaxy, lacking prominent spiral arms or distinct features indicative of active star formation. A slight asymmetry or minor disturbance may be present in the outer regions, hinting at a possible past interaction or minor merger event.
