The galaxy presents an overall elliptical morphology. It appears relatively smooth in structure, lacking prominent spiral arms or distinct features often associated with disk galaxies. The light distribution suggests a centrally concentrated profile, with the brightest region located at the core. The color index indicates a redder overall color, implying a dominant population of older stars and a lower rate of ongoing star formation within the galaxy. There is a faint visual indication of interaction with a secondary object, potentially resulting in a minor disturbance of morphology.
