The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright core. Moving outward, the luminosity gradually decreases, lacking any distinct spiral arm structures. The overall color appears slightly blue-green in the center, shifting toward redder hues in the outer regions, potentially indicating an older stellar population in the outskirts. A minor visual disturbance, such as a faint tidal tail or distorted shape, is not obviously apparent, however there are indications of a potential minor interaction or disturbance on the lower left side of the galaxy. Based on the object's color profile it has a moderate rate of star formation for its stellar mass.
