The galaxy appears as a relatively smooth, rounded object with a concentrated central region. There is a noticeable color gradient, shifting from a yellowish-white core to a more reddish-orange outer halo. No distinct spiral arms or bar structures are discernible. Faint hints of asymmetry are observed in the outer regions, possibly indicating a minor gravitational interaction or past merger event. The overall morphology suggests an elliptical or lenticular galaxy with a substantial population of older stars, consistent with relatively low star formation activity.
