The galaxy presents a somewhat elliptical morphology, displaying a noticeable bulge component that appears relatively smooth and concentrated towards the center. The disk appears somewhat blurred but shows at least one feature that may be an arm. Dust appears to be present in the disk. The central region exhibits a yellowish hue, potentially indicating an older stellar population. Extending outward from the central region, a bluer component is present, possibly signifying regions of more recent star formation. The galaxy does not appear to be undergoing any major merger activity, although there is a hint of a minor disturbance or interaction on one side, indicated by the color change in the disk. The galaxy's overall color suggests an intermediate stage of evolution, transitioning from a star-forming spiral to a more quiescent state.
