The galaxy presents as a single, relatively symmetrical, and concentrated object. It appears elliptical, with a high degree of smoothness. The galaxy exhibits a bright core, which is suggestive of a significant concentration of stars in the central region, such as a bulge. The overall color is yellowish-red, potentially indicating an older stellar population with lower ongoing star formation. The galaxy does not show any obvious signs of spiral arms or a well-defined disk structure within the limitations of the image quality. There are no obvious signs of tidal tails or disrupted morphology, pointing toward a lack of recent major mergers or interactions.
