The galaxy presents a generally smooth, rounded morphology, lacking prominent spiral arms or a distinct bar structure. Its light distribution appears centrally concentrated, with a gradual decrease in intensity toward the outer regions. The color is predominantly reddish-yellow, suggesting an older stellar population with fewer hot, young stars contributing significantly to the overall luminosity. There is a slight elongation to the shape, but it is not highly pronounced. No obvious signs of recent or ongoing major mergers are apparent, and the galaxy appears relatively undisturbed in its morphology.
