The galaxy presents as a flattened, disk-shaped structure oriented nearly edge-on to our line of sight. It exhibits a bright, concentrated central bulge, suggesting a significant population of older stars. The disk appears relatively smooth with no obvious spiral arm structures visible. The light from the disk fades gradually away from the central bulge in both directions, and displays a blue hue. The Sersic index value suggests that the galaxy is dominated by a de Vaucouleurs profile, associated with elliptical galaxies. The strong presence of the central bulge suggests it may be an S0 type galaxy.
