This galaxy appears to be a relatively compact, elliptical type, exhibiting a flattened, disk-like structure when viewed from our vantage point. The core region displays high luminosity and a bluish-white hue, suggesting a population of young, hot stars or an active galactic nucleus. The outer regions fade into a less concentrated halo, with a smoother, more diffuse light distribution. There's a hint of faint disturbance in the disk, possibly indicating minor interaction with another galaxy or past merger event. The galaxy overall has a smooth appearance in the outer edges of the disk, with a smooth transition from the disk to the edges of the galaxy. 
