The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a slightly elliptical morphology, appearing mostly rounded in shape. The central region displays a bright, concentrated core that gradually fades outward into a more diffuse halo. There is a suggestion of a disk-like structure, but no prominent spiral arms or bar are readily apparent. A faint blueish hue is visible in the outer regions, possibly indicating some degree of ongoing star formation, but it's subdued. There are no obvious signs of a major ongoing merger, but subtle disturbances may be present in the outskirts suggesting a prior interaction or accretion event. Overall, the galaxy appears as a transitional object, potentially in the process of evolving from a more active, disk-dominated system to a more quiescent, spheroidal form.
