The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated, bright central bulge with a surrounding, less luminous halo. The galaxy displays a slight elongation, deviating from a perfectly circular shape. There are no prominent spiral arms or dust lanes visible. Subtle color variations are present, with a yellowish-white core possibly indicating an older stellar population. A hint of bluer light appears towards the outer regions, perhaps suggesting some ongoing, but limited, star formation. The overall structure suggests a galaxy that is not currently undergoing significant merging activity, though subtle disturbances cannot be ruled out.
