The galaxy presents as a relatively smooth, elliptical form. Its core exhibits high luminosity, with a gradual decrease in brightness toward the outer regions. The overall color appears to be a yellowish-white hue, suggesting an older stellar population with relatively low ongoing star formation. The structure is generally undisturbed, lacking any prominent spiral arms or obvious signs of ongoing mergers or tidal interactions. The morphology is consistent with that of an elliptical galaxy with a high degree of central concentration. There are no obvious dust lanes or prominent features indicative of a younger stellar population.
