The galaxy appears to be largely elliptical, with a smooth, centrally concentrated luminosity profile. The core exhibits a bright, almost saturated glow, likely indicative of a high stellar density and possible active galactic nucleus. The overall shape is somewhat elongated. Faint, diffuse light extends outward from the central region, but there is no apparent spiral structure or well-defined disk. There are no obvious signs of a major ongoing merger. Weak evidence of a minor disturbance is suggested by very slight asymmetry in the outer regions, with possibly a faint tidal tail.
