The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is circular in appearance. The light distribution suggests a spheroidal morphology, lacking prominent spiral arms or a well-defined disk. The central region exhibits a significantly higher surface brightness than the outer regions, indicating a concentrated nucleus or bulge. The color appears somewhat redder, especially towards the center. This suggests an older stellar population dominates, with relatively little ongoing star formation. There is slight asymmetry in the outer isophotes, which may be indicative of minor tidal interactions or disturbances, although no major merger events are obviously apparent in the image.
