The galaxy presents as a slightly elongated, elliptical structure. It exhibits a smooth, featureless morphology across the majority of its visible extent. A subtle color gradient is observed, with a slightly bluer hue at its center, transitioning to redder tones in the outer regions. This color gradient suggests a potential variation in stellar populations, possibly indicating ongoing or recent star formation in the central region with older, redder stars populating the outskirts. There is a hint of a faint disk, although ill-defined, around the central bulge. No clear signs of major mergers or significant tidal disturbances are evident in the immediate vicinity of the galaxy. The galaxy does not appear perfectly round, with its shape being somewhere in between round and cigar-shaped.
