This galaxy exhibits a generally smooth morphology, with a high degree of central concentration. Its overall shape is elliptical, deviating slightly from perfectly round, leaning towards an intermediate ellipticity. The galaxy's color profile suggests an aging stellar population, dominated by older, redder stars, particularly towards the central bulge. A subtle disk-like structure may be present but it does not dominate the image, if it exists at all. There are no apparent signs of spiral arms or significant dust lanes. No strong evidence of ongoing or recent major merging activity is observed, though minor irregularities might suggest past interactions. The galaxy appears to be relatively quiescent in terms of star formation, as indicated by the lack of bright blue regions associated with young, massive stars.
