The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that is visibly brighter and has an orange hue, which is indicative of an older stellar population. The outer regions of the galaxy fade into a greenish color, suggesting the potential presence of ongoing, albeit suppressed, star formation or a population of intermediate-age stars. The galaxy appears undisturbed, displaying no major signs of tidal interactions or mergers. There is a subtle hint of a disklike shape and possibly slight irregularities in the outer envelope that suggest minor asymmetries. Overall, the galaxy seems to be a massive system, consistent with being a mature and relatively quiescent galaxy in its evolutionary stage.
