The galaxy presents an elliptical morphology with a high degree of central concentration. The central region appears yellowish-white, indicative of an older stellar population. The outer regions exhibit a fainter, bluer hue that surrounds the central region, possibly indicating more recent, although relatively low, star formation activity in the galaxy's disk. Overall, the galaxy appears to have a fairly smooth and regular structure, with only subtle indications of minor disturbances in its outer regions.
