The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a central concentration of light, likely representing a galactic bulge or core. The overall color profile leans towards warmer hues, with a yellow-orange tint, suggesting a population of older stars and relatively lower rates of on-going star formation. There is a subtle extension along one axis, suggesting the galaxy is not perfectly spherical and may be either a flattened elliptical or a lenticular type. No distinct spiral arms or dust lanes are visible. There are no merging features or major disturbances easily observed.
