The galaxy presents as an elliptical or lenticular type based on its smooth, largely featureless appearance. Its morphology is dominated by a centrally concentrated bulge that diminishes in brightness towards the edges. The galaxy displays a primarily round shape. There is no obvious spiral arm structure. There is no obvious merger activity or tidal disturbance. The color profile suggests an older stellar population, with redder hues concentrated in the central bulge and a gradual shift towards slightly bluer tones in the outer regions. The overall symmetrical shape of the galaxy indicates a relatively settled and undisturbed evolutionary history. 
