The galaxy presents as a relatively smooth, elliptical-like structure. There is a distinct central bulge exhibiting a yellowish-white hue, suggestive of an older stellar population. The galaxy shows a slight elongation, deviating from a perfectly circular form; it can be approximated as moderately in-between, showing no strong spiral arms or organized structures. A subtle transition to a bluer color is observed in the outer regions, hinting at a potential presence of younger stars or ongoing, albeit limited, star formation. There is no evidence of major disturbances from interactions with other galaxies or ongoing mergers. The galaxy appears generally isolated and unperturbed.
