The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or dust lanes. The light profile indicates a gradual decrease in intensity from the core outwards. There is a slight elongation to the shape, deviating minimally from a perfect circle, suggesting a possible classification between round and cigar-shaped. There is no apparent indication of on-going major merger activity; however, a subtle irregularity hints at a minor interaction or disturbance. The color indices imply a moderate stellar population, with no unusually high concentrations of extremely young, blue stars nor ancient red stars. The inferred size suggests that this is a massive galaxy.