The galaxy presents a smooth, elliptical morphology. Its color profile indicates a higher concentration of redder hues, with gradients toward a blue-greenish hue near the galaxy's outer edges. No distinct spiral arm structure is discernible, however some faint hints of asymmetrical form could suggest either a past or ongoing minor interaction. This indicates a significant fraction of older stellar populations. The central region appears more concentrated and luminous than the periphery, indicative of a possible central bulge.
