The galaxy appears as a relatively smooth, elliptical-shaped object. It presents a bright, concentrated central bulge, which suggests a high density of stars in the core. The galaxy exhibits a gradual fading in luminosity from the center outwards, lacking sharply defined spiral arms or prominent dust lanes. The overall color of the galaxy appears yellowish-white, indicating an older stellar population, potentially with limited ongoing star formation. There is a hint of elongation in the galaxy's shape, leaning toward a more cigar-shaped form rather than being perfectly circular. There is no apparent evidence of major mergers or tidal disturbances affecting the galaxy's morphology. The outer regions of the galaxy are indistinct, lacking clear spiral structure or disk features.
