The galaxy presents a generally smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, suggesting a high stellar density and possible presence of an active galactic nucleus. The luminosity appears to diminish gradually from the center outwards, fading into a diffuse halo. The disk is tilted relative to our line of sight, and is approximately 3.6 Kpc across. There is weak color variation across the galaxy, but there is a hint of blue light in the disk indicating some active star formation. There are no signs of major mergers or tidal disturbances.
