The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features. The color gradient transitions from a yellowish-white core to a redder outer halo. The smooth profile suggests a population of older stars, and the lack of distinct features indicates a quiescent or passive star formation history. The galaxy exhibits a somewhat rounded, though slightly elongated, shape. No significant signs of tidal disturbances or ongoing merger activity are evident in the immediate vicinity. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
