The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a somewhat spherical shape, with a hint of elongation along one axis, but generally appears quite round. The color profile displays a gradient, transitioning from a yellowish-white core to a reddish-orange periphery. The core region appears relatively bright, indicative of a high stellar density or perhaps ongoing active galactic nucleus activity. The outer regions of the galaxy appear diffuse, suggesting a gradual decrease in stellar population density. There is no distinct evidence of spiral arms or a well-defined disk structure. Subtle color variations in the outer regions may indicate variations in the stellar populations. There is no clear evidence of major tidal disturbances, though some slight asymmetry could hint at a minor interaction or recent accretion event.
