This galaxy exhibits a generally smooth morphology. It appears elliptical, with a bright central bulge. There is a slight extension of light around the central bulge, which could possibly indicate a very faint disk component but no distinct spiral arms are visible. The color gradient appears to be redder in the central regions, becoming slightly bluer towards the outer edges. There is no apparent major disturbance or ongoing merger activity. The galaxy's light distribution is not perfectly circular, but leans more toward an "in between" rounded shape. This suggests a classification between a perfectly round and an elongated ellipsoid galaxy. The overall color suggests an older stellar population.
