The galaxy presents a smooth, elliptical morphology. It appears largely featureless, lacking discernible spiral arms or a prominent dust lane. The color gradient exhibits a central concentration of yellowish light, indicating a likely population of older, redder stars in the core. This coloration gradually fades into a more diffuse, slightly bluer halo, suggesting the presence of some younger stellar populations in the outer regions, though to a limited extent. There's a subtle hint of a deviation from perfect circularity, perhaps indicating a slight degree of ellipticity. There is no evidence of any significant ongoing merger activity or major tidal disturbances affecting its structure. The galaxy appears to be relatively isolated and undisturbed.
