The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears largely homogenous in color. The radial intensity profile suggests a gradual decline in luminosity from the center outwards. The overall color appears to be yellowish, possibly indicating an older stellar population with suppressed star formation. There is a hint of a faint disk-like structure extending beyond the central bulge, though the smoothness of its appearance makes it difficult to definitively categorize as a spiral galaxy. The galaxy appears relatively undisturbed with no apparent major merging events. Minor disturbances cannot be ruled out given the image quality.
