The galaxy presents as a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, with a color profile tending towards redder wavelengths. The overall form is noticeably rounded, displaying minimal deviations from a circular shape. There is no apparent major disturbance to its structure, nor evidence suggesting an ongoing merger with another galaxy. Subtle signs of possible minor disturbances may be present but are not conclusive from this image alone. The galaxy shows a distinct lack of prominent spiral arms or well-defined disk features, supporting its classification as an elliptical galaxy. The overall appearance is consistent with an evolved stellar population, potentially indicating relatively low levels of current star formation activity.
