The galaxy presents an elliptical morphology, exhibiting a generally smooth appearance with a central bulge region. The galaxy's color profile suggests a concentration of older stellar populations in the core, shifting toward bluer hues in the outer regions, hinting at ongoing or recent star formation activity. There is a subtle hint of a disk-like structure in the galaxy. The isophotes reveal an elongated shape, possibly classifying the galaxy as an elliptical. No strong tidal features or obvious signs of a major merger are apparent. The galaxy is not perfectly symmetrical, presenting a slight warp. Overall, the object presents an elliptical galaxy with indications of modest star formation.
