The galaxy presents as a relatively smooth, elliptical object. It exhibits a concentrated central bulge with a gradual fading towards its outer edges. The color profile suggests a predominantly older stellar population, indicated by the reddish-orange hue of the bulge. A subtle greenish tint towards the outer regions hints at some, albeit minimal, ongoing star formation activity. The galaxy appears undisturbed with no signs of tidal tails or major mergers, implying a stable, relaxed system. Its morphology suggests it is likely an evolved system, having exhausted much of its gas reservoir and star-forming capabilities.
