The galaxy appears as a centrally concentrated, yellowish-white object. Its morphology is largely smooth and elliptical with no prominent disk structure visible. The light is fairly uniform, with a slightly brighter core region indicative of a possible central bulge. There seems to be some evidence of minor tidal disturbances or perhaps faint, diffuse features surrounding the main body of the galaxy, particularly towards the lower region of the galaxy. The smooth light profile suggests that the galaxy has undergone significant evolutionary processes. The colour suggests an older stellar population. Star formation appears to be relatively low, likely due to the lack of gas reservoirs to actively produce stars.
