The galaxy presents a smooth, elliptical morphology. Its light profile appears centrally concentrated, exhibiting a bright, diffuse core that fades gradually outward. There is little indication of spiral arms or a prominent disk structure, suggesting a relatively evolved system. Color gradients within the galaxy are subtle, with a general trend toward bluer hues in the outer regions and redder hues closer to the center. The galaxy exhibits a relatively high degree of roundness, with no obvious signs of tidal disturbances or ongoing mergers. The overall impression is that of a quiescent galaxy with a relatively low rate of star formation, primarily composed of an older stellar population.
