The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, with a high degree of central light concentration and a smooth gradient outwards. The color profile suggests an older stellar population, as indicated by the yellowish-red hue dominating the galaxy's core and diminishing outwards, with a bluer halo of more recent star formation. The galaxy exhibits minimal evidence of spiral arm structures or significant dust lanes, hinting at a relatively low star formation rate. There is no apparent major interaction or merger activity observed, and the overall symmetry is intact.
