The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a prominent bulge component which appears nearly spherical in projection. The overall light distribution suggests a high degree of rotational symmetry, showing no pronounced bar or spiral arm structures within the available resolution. The central region appears brighter and more yellow, suggesting an older stellar population and/or increased dust obscuration. The outer regions of the galaxy show a subtle color gradient, transitioning towards a bluer hue, potentially indicating the presence of younger stars. There is no evidence of any ongoing major mergers or significant tidal disturbances in the image. The galaxy seems to be a relatively undisturbed system, potentially a lenticular or elliptical galaxy at an approximate distance corresponding to a redshift of approximately 0.119.
