The galaxy presents as an elliptical morphology, appearing largely spheroidal with a smooth light distribution and no discernible spiral arm structure. The color gradient exhibits a central concentration of light with a warmer, reddish-orange hue, suggesting an older stellar population dominating the core. Moving outward from the core, the color shifts towards a slightly cooler, greenish-yellow tinge in the outer regions. This color difference could indicate the presence of a younger stellar population or increased metallicity in the outer regions, though this is not definitively observable from the image alone. There is no evidence of significant dust lanes or prominent star-forming regions. The overall structure is quite regular, with no major distortions or signs of ongoing mergers readily apparent. The galaxy appears relatively quiescent in terms of star formation activity.
