The galaxy presents as a relatively compact, elliptical or lenticular structure. Its morphology appears largely smooth, with a high degree of central concentration and a gradual decrease in surface brightness outward from the core. The galaxy exhibits a subtle elongation, appearing somewhere between a spheroidal and disk-like structure. The color profile suggests a predominantly older stellar population, with a bias towards redder wavelengths throughout the galactic body. There is no clear evidence of spiral arms, dust lanes, or significant ongoing star formation within the visible region. There might be only minor disturbances, or maybe no disturbances at all.
