The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The central region exhibits a bright, yellowish-white core, potentially indicating an older stellar population. The galaxy's overall shape is more elongated than circular, appearing somewhat disc-like but lacking any discernible spiral arm structure. The colors shift subtly from the core outwards, becoming slightly redder, this suggests that the outer regions may contain a lower proportion of young, blue stars. There is no apparent indication of significant ongoing star formation within the galaxy based on visual inspection. The galaxy appears relatively undisturbed, lacking evidence of major mergers or tidal interactions with neighboring galaxies, although the outer edges are somewhat fuzzy and indistinct.
