The galaxy presents as a generally smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that appears yellowish in color. The light appears to gradually diffuse from the center outwards, forming a halo. This halo is less luminous than the central bulge and shows a slight bluer color. The round shape suggests minimal rotational support, typical of early-type galaxies, and indicates a potentially older stellar population. There is no evidence of spiral arms, dust lanes, or significant disturbances in the galaxy's morphology, suggesting the absence of active star formation or recent major merger events.
