The galaxy presents a largely smooth and elliptical morphology. A central bulge, exhibiting a yellowish hue, dominates the structure and indicates a concentration of older stellar populations. Fainter, bluer emissions extend outwards from the core, suggesting the presence of some younger stars and possibly ongoing, albeit subdued, star formation within the galaxy. There appears to be no distinct spiral arm structure or significant dust lane features, consistent with an evolved system. Overall, the galaxy appears relatively undisturbed, showing no strong evidence of recent major mergers or tidal interactions.
