The galaxy presents as a smooth, elliptical morphology. It exhibits a concentrated central bulge with a radial color gradient, transitioning from a yellowish-white core to a fainter, bluer outer halo. There is a slight asymmetry in the outer regions, with a possible faint extension on one side, suggesting a minor gravitational disturbance or interaction, though a recent merger is unlikely. The overall shape is generally round, with only a slight deviation toward an elongated form. The galaxy's color index suggests a population of older stars dominating the core, while the bluer halo indicates the presence of a younger stellar population. Overall, it has a medium mass and star formation rate compared to other galaxies.