The galaxy presents a largely smooth, elliptical morphology. There appears to be little to no discernible disk structure, with a central, brighter region that fades gradually outward. The core appears yellowish, potentially indicating an older stellar population and/or dust obscuration. The outer regions exhibit a bluer hue, suggestive of more recent star formation, though this is less pronounced than the core color. There are no obvious signs of significant tidal disturbances or ongoing major mergers, although a subtle asymmetry in the outer halo cannot be ruled out as a minor interaction. The overall roundness suggests a classification towards the rounder end of the elliptical spectrum, showing minimal elongation. The galaxy doesn't appear to be particularly compact, indicating a degree of spatial extent.
