The galaxy presents as a centrally concentrated, smooth object, with a mostly featureless structure. The morphology appears to be generally elliptical, though perhaps slightly elongated, without any obvious spiral arm structure. There is a very slight suggestion of a disc component, based on the color gradient from core to the outer edges. The galaxy's color is slightly on the redder side, indicating an older stellar population, but with a small amount of blue color also present, indicating star formation is not entirely absent. There is no clear evidence of any major ongoing merger or tidal disturbance, though a very slight asymmetry could be interpreted as evidence of minor interaction. 
