The galaxy appears to be an elliptical galaxy, exhibiting a smooth, relatively featureless morphology. It is centrally concentrated, with the light intensity gradually decreasing outwards from the core. The galaxy displays a slight elongation, suggesting it is not perfectly spherical. The primary axis appears to be rotated about 160 degrees from vertical. The color appears to be dominated by older stellar populations, indicated by a yellowish-red hue. There are no prominent spiral arms or dust lanes visible. The overall appearance suggests a mature galaxy that has largely exhausted its gas supply and has a low star formation rate.
