The galaxy exhibits a roughly elliptical morphology. The central region presents a bright, concentrated core, suggesting a substantial concentration of stars or potentially an active galactic nucleus. A faint, diffuse halo surrounds the core, gradually fading into the background. The light distribution in the halo is not uniform, showing subtle variations in intensity. There are hints of asymmetry in the outer regions, possibly indicating past or ongoing gravitational interactions. Some redder regions are visible, potentially indicative of dust lanes, redder, older star populations, or star formation. The edges of the galaxy have a patchy blue fringe, which could be related to some artifacts.
