The galaxy presents a smooth, elliptical morphology with a bright, concentrated core. The light distribution appears relatively uniform, lacking distinct spiral arm structures or prominent dust lanes. The galaxy exhibits a slight elongation, with an ellipticity that suggests a deviation from a perfectly circular shape. The color profile indicates a redder hue in the central bulge, transitioning to a slightly bluer color in the outer regions. This color gradient potentially indicates older stellar populations concentrated in the core and younger stars populating the outskirts. There are no obvious signs of active galactic nuclei activity or significant starburst regions visible in this image.
