The galaxy presents as a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a radial falloff in luminosity, lacking distinct spiral arm structures or prominent dust lanes. The core region appears yellow-red, suggesting an older stellar population dominating this area. The outer regions are a gradient of green that might suggest recent star forming regions. The overall color suggests a galaxy transitioning from a star-forming state to one where star formation is diminished. There is no visual evidence of ongoing major mergers or tidal disturbances.
