The galaxy presents as a relatively smooth, centrally concentrated object with an overall elliptical morphology. It displays a gradual radial falloff in surface brightness, lacking prominent spiral arm structures or distinct features typically associated with late-type galaxies. The color profile appears predominantly redder, suggestive of an older stellar population and potentially lower ongoing star formation activity. There is a slight elongation visible, hinting at a possible deviation from perfect sphericity, but no indications of major mergers or tidal disturbances are apparent. The galaxy exhibits a round shape and no clear signs of merging.
