The galaxy appears to be a relatively smooth, elliptical or lenticular system. It exhibits a centrally concentrated light profile, with a gradual decrease in surface brightness from the core outwards. The galaxy has a generally round morphology, lacking any prominent spiral arm features or a distinct disk component. There is a hint of some disturbance or minor irregularity in the morphology, but it is largely subtle. The color suggests an older stellar population, potentially dominated by evolved stars. The overall structure appears relatively undisturbed, with no signs of ongoing major merger activity.
