The galaxy presents as a relatively smooth, elliptical morphology. The central bulge appears prominent, with a high degree of radial symmetry and a lack of readily discernible spiral arm structures. The light distribution indicates a spheroidal shape, appearing nearly circular on the plane of the sky. The galaxy exhibits a color gradient, transitioning from a yellowish core to more reddish outer regions. There is little evidence of significant dust lanes or active star formation regions within the galaxy. The overall appearance is consistent with a passively evolving galaxy, dominated by an older stellar population.
