The galaxy appears as a centrally concentrated elliptical object. It exhibits a generally smooth, featureless morphology, with a slight elongation. The light distribution suggests a centrally dominant bulge component. The galaxy displays a color gradient, transitioning from a more yellowish-white core to a redder outer halo. This suggests a stellar population gradient, with older, redder stars more prevalent in the outer regions. It is possible that the object is currently undergoing a minor merger, or tidal interaction event with a smaller companion galaxy, evidenced by the overall disturbed appearance.
