The galaxy appears as a centrally concentrated object with a smooth, generally elliptical morphology. Its color profile suggests a predominantly older stellar population, exhibiting a reddish hue. There is little indication of distinct spiral arm structures or active star formation regions within the observable light. The galaxy displays a high degree of circularity and does not seem to be undergoing any major merger events or significant tidal disturbances. There might be a hint of an extended halo or diffuse light surrounding the main body, but it is faint and not well defined. Overall, the galaxy presents as a relatively undisturbed elliptical or lenticular system.
