The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. There is a noticeable color gradient, shifting from a redder core to a slightly bluer outer halo, potentially indicating younger stellar populations in the outer regions. The galaxy appears relatively undisturbed, showing no significant signs of tidal interactions or ongoing major mergers. It seems fairly round, displaying only a slight deviation from perfect circularity. Overall, the light distribution suggests a relaxed system dominated by older stellar populations in the core, with some ongoing star formation activity at its periphery.
