The galaxy appears to be a relatively smooth, elliptical type galaxy. It exhibits a concentrated central bulge. The galaxy has a generally rounded morphology with a smooth light distribution, lacking prominent spiral arms or distinct features. There is a slight elongation to the galaxy’s shape, but it is predominantly circular. Color gradients suggest a possible variation in stellar populations, with a yellowish hue indicating older stars. There are no readily apparent signs of active galactic nuclei activity or significant dust lanes. The lack of significant disturbance in the galaxy's structure suggests it is not undergoing a major merger or interaction. Overall, it presents as a quiescent, evolved system.
