The galaxy presents as a somewhat elongated, disk-shaped structure with a bright central bulge. The bulge appears relatively smooth and featureless. The disk shows a subtle blue tint, suggesting the presence of younger stars. There is a faint, extended halo surrounding the main body of the galaxy, but details are difficult to discern. The overall morphology suggests an intermediate-type spiral galaxy, although the lack of clearly defined spiral arms leans towards a lenticular classification. The disk exhibits a degree of asymmetry.
