The galaxy presents as a relatively smooth, elliptical or lenticular system. The central bulge exhibits a yellowish hue, indicative of an older stellar population. There is a subtle, bluer disk component, suggesting ongoing, albeit subdued, star formation. The galaxy appears largely undisturbed, with no readily apparent signs of major mergers or significant tidal interactions. It has an intermediate apparent roundness. Overall, the galaxy shows characteristics consistent with a massive, evolved system.
