The galaxy presents as a fairly smooth, centrally concentrated object, likely an elliptical. It exhibits a spheroidal morphology with a high degree of circularity, showing only a slight elongation. The galaxy's color profile suggests an older stellar population, appearing redder in overall color. Star formation appears relatively low. There's no clear evidence of spiral arms or a prominent disk structure. No obvious signs of recent or ongoing major merging events are discernible. The galaxy's surface brightness diminishes gradually from the core to its outer regions.
