The galaxy presents a smooth, elongated morphology, consistent with an elliptical or lenticular type. Its color profile indicates a redder overall population, with a subtle concentration of light toward the center. There is no visible evidence of spiral arms or a prominent disk structure. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal disruptions. The overall light distribution is fairly even, with a gentle gradient outward from the core, which suggests that it is nearing a more compact shape. There is a slight asymmetry in the galaxy’s elongated form, though this could be the result of viewing angle.
