The galaxy presents a generally smooth, elliptical morphology, exhibiting a concentrated central bulge that appears nearly spherical. There is little evidence of spiral arm structure or distinct features. The galaxy displays a color gradient, transitioning from a bluer hue in the core region to redder colors towards the outer edges, suggesting a potential decline in recent star formation activity as a function of radial distance. There is no sign of major merger activity in the form of tidal tails or disturbed morphology. The galaxy appears relatively undisturbed and isolated.
