The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light profile. There is a noticeable color gradient, shifting from a redder hue in the central core region to a bluer component in the outskirts, suggesting a potential age or metallicity difference between these regions. The galaxy is relatively symmetrical, with no distinct spiral arm structures or prominent dust lanes visible. Its overall appearance is relatively undisturbed, indicating a lack of major recent merger activity. The extended halo appears diffuse, lacking sharp boundaries. There are no obvious signs of intense star formation within the galaxy when examining its color.
