The galaxy presents as a relatively smooth, lenticular-like structure. It is not perfectly round, exhibiting a slightly elongated, cigar-shaped morphology. A disk is faintly visible. The galaxy's color appears to be generally bluish, which could indicate a population of younger stars. There are no obvious signs of major mergers or significant tidal disturbances. The light distribution is concentrated in the center, which could suggest a dense galactic nucleus. The galaxy has moderate star formation.
