The galaxy presents an elliptical morphology, exhibiting a smooth, centralized luminosity profile. The light distribution suggests a concentration of older stellar populations towards the galactic core, indicated by the reddish hue. A subtle transition towards bluer colors can be observed in the outer regions, potentially indicative of ongoing or recent star formation activity, albeit at a relatively low rate. There is no apparent evidence of spiral arm structures or a distinct disk. The galaxy appears relatively undisturbed with a slight hint of asymmetry, though not indicative of a major merger event. The object's apparent roundness suggests a minimal inclination relative to our line of sight.
