The galaxy presents a largely smooth morphology with a highly concentrated central bulge. The color profile suggests an older stellar population, with a yellowish-white core that likely hosts a supermassive black hole. A fainter, bluish halo surrounds the bulge, potentially indicative of more recent, though limited, star formation in the outer regions. The galaxy appears nearly spherical in shape, exhibiting minimal evidence of a disk structure or spiral arms. There is little evidence of recent merger activity or significant tidal disturbances, and it seems to be an isolated elliptical galaxy.
