The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The light profile appears centrally peaked, exhibiting a gradual decrease in surface brightness moving outwards from the core. The galaxy displays a yellowish color, hinting at an older stellar population, with relatively minimal evidence of ongoing, vigorous star formation, although some blue light is present. There is no clear indication of spiral arms or a distinct disk-like morphology. The overall appearance suggests a galaxy that is evolved, with a spheroidal shape and a predominantly old stellar population. There is no strong evidence of significant tidal interactions or recent merger activity. The overall morphology is consistent with an elliptical galaxy that has largely exhausted its supply of gas for star formation.
