The galaxy appears as a luminous, centrally concentrated object with a generally smooth morphology. The galaxy exhibits a round shape, with only minor deviations from circular symmetry.  A slight yellow-orange hue dominates the central region, suggesting a population of older stars.  There are no prominent spiral arm structures or dust lanes visible in this image, indicating that the galaxy is likely an elliptical galaxy. The system does not appear to be currently undergoing a major merger, although very minor irregularities in the outer regions cannot be completely ruled out at this resolution.  The galaxy exhibits significant luminosity. Based on the observed color and lack of discernible features, star formation activity appears low, but may be present at low levels within the galaxy.
