The galaxy presents as a relatively smooth, elliptical morphology. There is an extended halo of light surrounding what appears to be a central bulge. The color gradient suggests an aging stellar population; yellowish-white at the core shifting toward red at the periphery. A possible minor tidal disturbance is suggested on the right side, as there is a separate red region that appears associated with the main body of the galaxy. This secondary object could be either a smaller, interacting companion or a region of enhanced star formation, likely a region of lower mass. No significant dust lanes or spiral arm structures are discernible. The overall appearance is consistent with a galaxy that has undergone significant evolution, with a relatively low star formation rate.
