The galaxy appears to be a relatively smooth, elliptical system. It has a moderate concentration of light toward the center, indicating a bulge component, though without discernible spiral arms or a distinct disk. The galaxy's color is broadly consistent with an older stellar population, potentially with ongoing, but low-level star formation. Its overall shape is somewhat elongated, though it leans more towards a spheroid, suggesting a dynamically relaxed system. There may be a minor gravitational interaction occurring, with some asymmetry in the galaxy's halo, but no definitive major merger events can be identified.
