The galaxy presents a relatively smooth, elliptical morphology with no discernible spiral arms or bar structure. The central region exhibits a brighter, more concentrated luminosity profile, indicative of a galactic bulge. The galaxy appears somewhat rounded, with the light distribution gradually fading towards its outer edges. There is a hint of minor disturbances or asymmetries in the outer regions of the galaxy. No significant dust lanes or active star-forming regions are readily apparent. Overall, the galaxy appears to be relatively quiescent in terms of star formation activity.
