The galaxy presents as a centrally concentrated object with a moderately luminous core. The light distribution appears relatively smooth, suggesting a predominantly elliptical morphology. The isophotes exhibit a generally rounded form, with a slight deviation towards an intermediate ellipticity. There is a subtle color gradient, transitioning from a yellower central region to a bluer outer halo. No distinct spiral arm structures or significant dust lanes are visible, nor are any obvious signs of a major merger event, though a minor disturbance cannot be ruled out.
