The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, relatively featureless appearance. It exhibits a color gradient, transitioning from a yellowish-white core to a slightly redder periphery. The observed light distribution suggests a spheroidal morphology, lacking prominent spiral arms or a distinct disk component. There is no visible indication of ongoing major mergers or significant tidal disturbances in this image. The overall roundness and the smooth light profile indicate a system dominated by an older stellar population. Evidence suggests that star formation activity is relatively low, possibly due to the consumption of gas or the influence of environmental factors.
