The galaxy appears to be a relatively smooth, elliptical system. The light distribution is concentrated towards the center, indicating a prominent bulge. There is a slight elongation, though the overall shape is generally round. The core exhibits a yellow-orange hue, possibly indicating an older stellar population and/or dust obscuration. The outer regions of the galaxy fade into a bluish-green color, which could represent younger stars forming or a contribution from background light. There are no distinct spiral arms or other prominent features that would suggest recent major mergers or active star formation throughout the system. The lack of any visible tidal features or neighboring galaxies suggests that it is a relatively isolated galaxy.
