The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears bright and yellowish-white. The light from the galaxy is relatively uniform, suggesting an older stellar population, potentially dominated by Population II stars with lower rates of current star formation. The galaxy's shape appears more round than elongated. There is no strong evidence of spiral arms, prominent dust lanes, or other distinct morphological features such as tidal tails, or signs of a major merger event based on what is visible in the image. The smooth appearance and color profile hint at a relatively evolved system. There is a very slight disturbance in the bottom right.
