The galaxy presents as a slightly elliptical, moderately luminous object. It exhibits a high degree of smoothness, with little apparent substructure or distinct features discernable. The central region displays a concentration of light, appearing nearly spherical and transitioning into a surrounding disk-like structure. The color profile suggests a population of older stars, indicated by the reddish hue in the core. Faint hints of bluer regions are scattered within the surrounding structure, potentially suggestive of more recent, though limited, star formation activity. There is no obvious evidence of spiral arms, a bar, or signs of a major ongoing merger event, although a slight asymmetry could indicate a minor gravitational interaction or disturbance.
