The galaxy presents a largely smooth, elliptical morphology. Its color profile indicates a concentration of older stellar populations, emitting strongly in the redder wavelengths. The core is a bright, concentrated region, suggesting a high density of stars and potentially a supermassive black hole actively accreting material. There are hints of disturbed morphology, which may be indicative of minor interaction or merging event. A faint disk could also be present. The spatial extent suggests a galaxy of considerable size. Overall, the galaxy appears to be a massive, relatively quiescent system undergoing little star formation currently.
