The galaxy appears to be a relatively smooth, centrally concentrated object, with a dominant, elliptical morphology. The core exhibits a yellowish hue, which could indicate an older stellar population. Extending outward from the central region, faint wispy structures are visible. These could be tidal features, potentially suggesting past or ongoing gravitational interactions with another galaxy. Overall, the galaxy's light profile fades gradually towards its edges. There is a slight hint of bluer light in the surrounding regions of the core, possibly indicating some ongoing low levels of star formation. The general characteristics point toward a galaxy that has largely ceased active star formation and is dominated by an aging stellar population.
