The galaxy presents as a centrally concentrated object, exhibiting a smooth, relatively featureless morphology. It appears largely elliptical in shape, with a slight deviation from perfect circularity. The light distribution suggests a dominant bulge component. There is a subtle color gradient, transitioning from a yellowish-white core to a reddish-tinged outer region. There is no clear evidence of spiral arms, bars, or significant dust lanes. The overall appearance indicates a relatively evolved system, consistent with an older stellar population. The object does not appear to be undergoing any major merging events or significant tidal disturbances.
