The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The overall shape is somewhat elliptical, appearing as an intermediate form between perfectly round and elongated. There is a noticeable color gradient, transitioning from a bright, yellowish core to a more subdued and reddish outer region. No prominent spiral arms or disk features are readily discernible in this image. There is a hint of a minor disturbance that could be the result of gravitational interaction with a smaller galaxy, or perhaps an active galactic nucleus. The central region dominates the light output, suggesting an older stellar population.
