The galaxy presents as a moderately luminous, elongated structure with a smooth appearance. There is a bright central bulge that dominates the light output, indicating a high concentration of stars in the galactic nucleus. The light appears relatively red-shifted, meaning the galaxy is likely at an intermediate distance. The overall color suggests an older stellar population. The shape is more elongated, with a subtle disk-like component that is faintly visible, although not well defined. There is no strong evidence of active star formation. No signs of tidal disturbances or ongoing mergers are observed. The galaxy displays a largely undisturbed morphology.
